203 research outputs found

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    Nisar Ahmad-Essay-The Role of Stereotypes in the Development of the Female Personality. pp. 1-2; M. Moazzam Zubair-Essay-By Love Serve One Another. pp. 3; Jehanzeb Anwar-Essay-A Great Escape. pp. 4-5; Ahmed Ilyas Butt-Essay-War: A Solution for Peace. pp. 6-7; Fatima Zahra-Essay-Proliferation of Electronic Media and Youth. pp. 8; M. Imran-Essay-Environmental Pollution and Our Responsibility. pp. 9; Muiz Junaid Khan-Essay-Intelligence. pp. 10; Safa Aleem-Essay-A Wake-up Call. pp. 11; Fareeha Tahir-Essay-Karo Kari: The Cruelest Reality in Pakistan. pp. 12-13; Adnan Farooqui-Essay-Democracy. pp. 14; Riaz Akbar-Essay-Politics: a Dirty Game or a Human Necessity? pp. 15-16; Mujtaba Chaudhry-Essay-Emancipation of Women. pp. 17; Adeel Riaz-Essay-The Unheard Miseries of Bonded Laborers. pp. 18-19; Nazeef Ishtiaq-Essay-Pakistan Today. pp. 20; Muhammad Adeel-Short Story-Broken Threads. pp. 21-23; Tehreem Fatima-Short Story-But Still. pp. 24; Naima Fatima-Short Story-Once Upon a Time. pp. 25-26; Syed Irfan Haider Shah-Short Story-By The Riverside, I Sat and Wept! pp. 27-28; Faiqa Javed-Short Story-Ghosts. pp. 29; M. Bilal Aslam-Short Story-A Mysterious Night. pp. 30-31; Sabrina Asim-Short Story-A Dismal Encounter. pp. 32; Umair Vahidy-Short Story-Uncertain Ambiguities. pp. 33-36; Jahanzaib Aslam-Interview-Jamsheed Marker. pp. 37-43; U. Vahidy, H. Aslam-Interview-Cecil Chaudhry's Interview. pp. 44-48; N. Ahmad, K. Shah-Interview-Muhammad Junaid. pp. 49-51; N. Ishtriaq, U. Vahidy-Interview-Qazi Laeeque Ahmed. pp. 52-56; S. Aleem, S. Ahmad-Interview-Bilal Bajwa. pp. 57-58; M. Mesam Ismail-Reflections-Loneliness. pp. 59; Haya Fatima-Reflections-I Love to Fantasize. pp. 60; Jahanzeb Anwar-Reflections-A Faith for the Faithless. pp. 61; Fizza Ali Shah-Reflections-Where Are We Heading To. pp. 62; Rabia Shad-Reflections-Need of Revolution. pp. 63; Mariam Iqbal-Reflections-An Extract from a Mother�s Diary. pp. 64; Ali Abbas-Reflections-Sense of Responsibility. pp. 65; Sabrina Asim-Reflections-Painting in Words. pp. 66; Dr. Waseem Anwar-Poetry-Reading Between Silences. pp. 67; Muhammad Adeel-Poetry-The Hand. pp. 67; Nauman Ahmad-Poetry-Fragrance, Piercing Through My Heart. pp. 68; Shumyila Imam-Poetry-Human Right. pp. 68; M. Y. Sandhu-Poetry-To the Mausoleum. pp. 69; Mumtaz Hussain Kherani-Poetry-The Real Inventor. pp. 69; Shakeel Fiaz-Poetry-God Almighty. pp. 70; Jahanzaib-Poetry-My Mother. pp. 70; Ahmed Ilyas Butt-Poetry-A Walk in the Park. pp. 70; Tajwar Ali Buber-Poetry-My Craze. pp. 70; Samra Zafarullah-Poetry-How can we Forget? pp. 71; Tanzeel Ahmad Khan Niazy-Poetry-My Daddy. pp. 71; Toqeer Ahamad Wazir Gilgity-Poetry-Heart and Mind. pp. 71; Faisal Nizami-Poetry-I am... pp. 71; Basit Zafar-Poetry-Lord! pp. 72; Nauman Ahmad-Poetry-I Try Reaching You. pp. 72; Muiz Khan-Poetry-Untitled. pp. 72; Warda Tahseen-Poetry-I am Not a Perfect Girl. pp. 72; Nisar Ahmed-Poetry-Chaos. pp. 73; Furqan Farukh-Poetry-I'll Die Another Day. pp. 73; Nisar Ahmed-Poetry-Secret Joy. pp. 74; Jahangir Jan Khokhar-Poetry-I Want To. pp. 74; Arman Ahmed-Poetry-On the Edge of Dreaming. pp. 74; Professor Arif Qureshi-Poetry-Mother, O' Dear Mother! pp. 74; Furqan Farrukh-Poetry-Love at First Sight. pp. 75; Faisal Karim Nomali-Poetry-Hazrat Muhammad (P.B.U.H.). pp. 75; Saad Akmal-Poetry-Laid Forgotten. pp. 75; Zamzam Rizvi-Poetry-A Lonely Island. pp. 76; Jahanzaib Aslam-Poetry-O My Beloved! pp. 76; Society Reports. pp. 77-80; [Urdu]. 80 p.Mr Jamsheed Marker. before page 37; Mr Cecil Chaudhry. after page 48; Qazi Laeeque Ahmed. after page 56; Mr Bilal Bajwa. before page 57; Presidents 2009-2010. after page 76; FCC Dramatic Club. before page 77; 20 pages covering different activities at FC, i.e. Alumni Reunion, Commencement, Honors Convocation, Drama, Class of 2010, Sports, Debates and Societies. after page 80; Professor Dr Agha Sohail. before page 7 Urdu section; Professor Dr Ehson Raza Khan. before page 15 Urdu sectio

    An extension of the localist representation theory: grandmother cells are also widely used in the brain

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    abstract: Based on considerable neurophysiological evidence, Roy (2012) proposed the theory that localist representation is widely used in the brain, starting from the lowest levels of processing. Grandmother cells are a special case of localist representation. In this article, I present the theory that grandmother cells are also widely used in the brain. To support the proposed theory, I present neurophysiological evidence and an analysis of the concept of grandmother cells. Konorski (1967) first predicted the existence of grandmother cells (he called them “gnostic” neurons)—single neurons that respond to complex stimuli such as faces, hands, expressions, objects, and so on. The term “grandmother cell” was introduced by Jerry Lettvin in 1969 (Barlow, 1995).View the article as published at http://journal.frontiersin.org/article/10.3389/fpsyg.2013.00300/ful

    Correspondence to Joseph E. Lowery from Asim Israel, August 29, 1986

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    A letter to Joseph E. Lowery from Asim Israel of the House of Israel requesting assistance in contacting Louis Stokes, Jesse Jackson, and Reverend Clay Evans to convince the Guyana government to release David Hill from prison. 1 page.The Atlanta University Center Robert W. Woodruff Library acknowledges the generous support of the Joseph & Evelyn Lowery Institute for Justice and Human Rights, the Joseph Echols Lowery Irrevocable Trust, and other donors in supporting the processing and digitization of Morehouse College's Joseph Echols and Evelyn Gibson Lowery Collection

    Förbättring av monteringsstation för plockningsroboten IRB 360 FlexPicker

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    This thesis is about product and process development. The thesis has been done at ABB Robotics AB in Västerås under 20 weeks with half study pace, which is equivalent to 15 higher education credits (15hp). Thesis purpose was to improve an assembly station for assembling of robot IRB 360. Problems at the assembly station are that there are some non-value-creating activities and assembling methods which correspond to low safety factor for workers. The focus of thesis was to investigate opportunities and to produce solid proposals for how to eliminate these problems. After a written contract with ABB AB, the work started with the planning with the company supervisor and Gantt Schema was created to schedule all steps for this project, to ensure during the process. The project has followed the methods described in the book "Produktutveckling konstruktion och design " by Karl T Ulrich & Steven D Eppinger. Product development tools like Quality function deployment (QFD), functional analysis, specification of requirement and Pugh's analysis matrix have been used in the development process. In the first phase of the project, observation and investigation has been performed to identify and analyse problems. In the later phases, ideas and concepts has created to solve the problems and achieve successful results. The result of the project is an improved material flow at assembling stations which eliminates nonvalue-creating activities and leads to better safety for workers. Another result of the project is an elimination of hand hammering at assembling station and for this purpose a new pressing tool has been developed for pressing down a seals around radial shaft in assembling process. The software Solidworks has been used to create a new 3D layout for the existing assembly station to understand and find the better solution for material flow. Solidworks is also used for doing Finite element method (FEM) analysis to validate the new developed pressing tool.Detta examensarbete handlar om produkt och processutveckling. Arbetet utfördes hos ABB Robotics AB i Västerås och bedrivs under 20 veckor långt på halvfart vilket motsvarar 15 högskolepoäng. Uppdraget är att förbättra en monteringsstation för plockningsrobot IRB360 FlexPicker. Problem på monteringsstation är att det sker icke värdeskapande aktiviteter, och monteringsprocess som leder till arbetsmiljöproblem. Arbetet fokus var att undersöka möjligheter och ta fram konkreta förslag att hur man kan eliminera dessa problem. Efter skriftligt kontrakt med ABB AB, arbetet började med planeringen med företaget handledare och skapades Gantt Schema. Projektet har följt metoderna som beskrivs i boken ”Produktutveckling konstruktion och design” av författare Karl T Ulrich & Steven D Eppinger. I utvecklingsprocessen har använt produktutvecklingsverktyg, några av dessa är QFD, funktionsanalys, kravspecifikation och Pughs analysmatris. I första fas av projekt gjorde undersökning och observation för att hitta och analysera problem. I senare faserna genererade koncepter för åtgärden och sedan vidare utvecklades utvalda koncept för nå framgångsrikt resultat. Resultatet av arbetet blev förbättrad materialflöde som eliminerar icke värdeskapande aktiviteter. Dessutom utvecklades fram ett nytt pressverktyg som eliminerar arbetsmiljöproblem. Mjukvaran Solidworks har använt för att skapa en ny layout för monteringsstation. Med hjälp av Solidworks gjordes FEM -analys (Finita elementmetoden) för att validera den nya pressverkty

    Responsible conduct and documentation of research: a standard operating procedure template that can be customized

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    If you have comments or suggestions for improvements, please direct these to the corresponding author, Catherine Hayward ([email protected]).This standard operating procedure (SOP) document was prepared as a template that individual researchers can customize for their own use. Prior to publication, this SOP underwent peer review by the McMaster University Faculty of Health Sciences Research Council. The Council has endorsed the publication of this SOP to encourage researchers to develop procedures that encourage best research practices and can be customized to meet specific needs. Should you decide to customize this SOP for your own use, please acknowledge the original authors, who include Ms. D’Andra Parker and Mr. Asim Soomro (graduate students in the Hayward laboratory). All items highlighted in yellow in the SOP must be customized. This procedure outlines the steps involved in proper recording keeping in the laboratory. This SOP applies any/all data generated while in the laboratory, and any/all the laboratory records

    Measuring microfinance access : building on existing cross-country data

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    Given the acknowledged need for a new effort to expand the set of available data on direct access to financial services, including a focus on access by those at low income, Honohan provides a selective review of the diverse sources of data that exist and considers how best to build on them. He proposes a basic framework within which to consider the analysis of the interesting questions: (1) How does access affect poverty and productivity? and (2) What hinders access? The author discusses existing and potential contribution of household and business user surveys, surveys of providers and their regulators, and surveys of experts, and assesses their relative strengths.Banks&Banking Reform,Environmental Economics&Policies,Health Economics&Finance,Poverty Assessment,Governance Indicators

    X-ray and gamma-ray timing of GRB 180720B, GRB 181222B, GRB 211211A, and GRB 220910A observed with Fermi and ASIM

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    We present a timing study of the gamma and X-ray observations and analysis of a sample of bright gamma-ray bursts (GRBs; i.e. GRB 180720B, GRB 181222B, GRB 211211A, and GRB 220910A), including the very bright and long GRB 211211A (a.k.a. kilonova candidate). They have been detected and observed by the Atmosphere–Space Interactions Monitor (ASIM) installed on the International Space Station (ISS) and the Gamma-ray Burst Monitor (GBM) onboard the Fermi mission. The early (T − T0≈ s) and high-energy (0.3–20 MeV) ASIM High Energy Detector (HED) and (150 keV–30 MeV) Fermi (BGO) light curves show well-defined peaks with a low quasi-periodic oscillation (QPO) frequency between 2.5 and 3.5 Hz that could be identified with the spin of the neutron star (NS) in the binary mergers originating these GRBs. These QPOs consist on the first detection of low-frequency QPOs (≤10 Hz) detected in magnetars so far. We also detect a strong QPO at 21.8 − 22 Hz in GRB 181222B together with its (less significant) harmonics. The low-frequency QPO would correspond to the signal of the orbiting NS previous to the final coalescence giving rise to the gravitational wave (GW) signal. © 2025 The Author(s).MCG acknowledges S. Xiao, M. Marisaldi, and A. Mezentsev for useful discussions and feedback. MCG acknowledges financial support from the Spanish Ministry project MCI/AEI/PID2023-149817OB-C31. RSR, YDH, MCG, SG, IPG, EJFG, RGB, MPV, and AJCT acknowledge financial support from the Spanish Ministry project PID2023-151905OB-I00 and the Severo Ochoa grant CEX2021-001131-S funded by MICIU/AEI/10.13039/501100011033. RG and SBP acknowledge BRICS grant DST/IMRCD/BRICS/PilotCall1 /ProFCheap/2017(G) for the financial support. RG and SBP also acknowledge the financial support of ISRO under AstroSat archival Data utilization programme (DS 2B-13013(2)/1/2021-Sec.2). RG was sponsored by the National Aeronautics and Space Administration (NASA) through a contract with ORAU. AJCT acknowledges support from the Junta de Andalucia Project P20 01068. MM, AL, AM, and NØ acknowledge financial support from the Research Council of Norway under Contracts 208028/F50 and 223252/F50 (CoE). This research has used data obtained through the HEASARC Online Service, provided by the NASA-GSFC, in support of NASA High Energy Astrophysics Programs. The NASA’s FGST (Fermi) mission is an astrophysics and particle physics partnership, developed in collaboration with the U.S. Department of Energy, along with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the United States. ASIM is a mission of ESA’s SciSpace programme for scientific utilization of the ISS and non-ISS space exploration platforms and space environment analogues. ASIM and the ASIM Science Data Centre are funded by ESA and by national grants of Denmark, Norway, and Spain.With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (CEX2021-001131-S).Peer reviewe

    Fixed point theorems for F- contraction mapping in complete rectangular M-metric space

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    [EN] In this paper, we prove a fixed point result for F- contraction principle in the framework of rectangular M-metric space. An example is also adopted to exhibit the utility of our result. Finally, we apply our fixed point result to show the existence of solution of Fredholm integral equation.Asim, M.; Mujahid, S.; Uddin, I. (2022). Fixed point theorems for F- contraction mapping in complete rectangular M-metric space. Applied General Topology. 23(2):363-376. https://doi.org/10.4995/agt.2022.17418OJS363376232M. Asadi, Fixed point theorems for Meir-Keeler type mappings in M-metric spaces with applications, Fixed Point Theory Appl. 2015 (2015), 210. https://doi.org/10.1186/s13663-015-0460-9M. Asadi, On Ekeland's variational principle in M-metric spaces, Journal of Nonlinear and Convex Anal. 17 (2016), 1151-1158.M. Asadi, M. Azhini, E. Karapinar and H. Monfared, Simulation functions over M-metric spaces, East Asian Math. J. 33 (2017), 559-570.M. Asadi, E. Karapinar and P. Salimi, New extension of p-metric spaces with some fixed-points results on M-metric spaces, J. Inequal. Appl. 18 (2014), 1-9. https://doi.org/10.1186/1029-242X-2014-18M. Asim, A. R. Khan and M. Imdad, Rectangular MbM_{b}-metric spaces and fixed point results, J. Math. Anal. 10 (2019), 10-18. https://doi.org/10.1186/s13660-019-2223-3M. Asim, S. Mujahid and I. Uddin, Meir-Keeler contraction in rectangular M-metric space, Topol. Algebra Appl. 9 (2021), 96-104. https://doi.org/10.1515/taa-2021-0106M. Asim, K.S. Nisar, A. Morsy and M. Imdad, Extended rectangular MrxiM_{rxi}-metric spaces and fixed point results, Mathematics 7 (2019), 1136. https://doi.org/10.3390/math7121136M. Asim, I. Uddin and M. Imdad, Fixed point results in MnuM_{nu}-metric spaces with an application, J. Inequal. Appl. 2019 (2019), 1-19. https://doi.org/10.1186/s13660-019-2223-3M. Aslantas, H. Sahin and D. Turkoglu, Some Caristi type fixed point theorems, TheJournal of Analysis 29 (2020), 89-103https://doi.org/10.1007/s41478-020-00248-8S. Banach, Sur les oprations dans les ensembles abstraits et leur application aux quations intgrales, Fund. Math. 3 (1922), 131-181. https://doi.org/10.4064/fm-3-1-133-181D. W. Boyd and J. S. W. Wong, On nonlinear contractions, Proc. Amer. Math. Soc. 20 (1969), 458-464. https://doi.org/10.1090/S0002-9939-1969-0239559-9A. Branciari, A fixed point theorem of Banach-Cacciopoli type on a class of generalized metric spaces, Publ. Math. 57 (2000), 31-37.S. K. Chatterjee, Fixed point theorems, C. R. Acad. Bulgare Sci. 25 (1972), 727-730.Lj. B. Ćirić, Generalized contractions and fixed point theorems, Publ. Inst. Math. 12 (1971), 19-26.Lj. B. Ćirić, A generalization of Banach's contraction principle, Proc. Amer. Math. Soc. 45 (1974), 267-273. https://doi.org/10.1090/S0002-9939-1974-0356011-2Z. Kadelburg and S. Radenović, Notes on some recent papers concerning F-contractions in b-metric spaces, Constr. Math. Anal. 1 (2018), 108-112. https://doi.org/10.33205/cma.468813R. Kannan, Some results on fixed points, Bull. Cal. Math. 60 (1968), 71-76. https://doi.org/10.2307/2316437S. Luambano, S. Kumar and G. Kakiko, Fixed point theorem for F-contraction mappings in partial metric spaces, Lobachevskii J. Math. 40 (2019), 183-188. https://doi.org/10.1134/S1995080219020094S. G. Matthews, Partial metric topology, Ann. N. Y. Acad. Sci. 728 (1994), 183-197. https://doi.org/10.1111/j.1749-6632.1994.tb44144.xA. Meir and E. Keeler, A theorem on contraction mappings, J. Math. Anal. Appl. 28 (1969), 326-329. https://doi.org/10.1016/0022-247X(69)90031-6G. Minak, A. Helvaci and I. Altun, Ćirić type generalized F-contractions on complete metric spaces and fixed point results, Filomat 28 (2014), 1143-1151. https://doi.org/10.2298/FIL1406143MH. Monfared, M. Asadi, M. Azhini and D. O'Regan, F(ψ,ϕ)-contractions for α-admissible mappings on m-metric spaces, Fixed Point Theory and Appl. 2018 (2018), 22. https://doi.org/10.30697/rfpta-2018-004H. Monfared, M. Azhini and M. Asadi, C-class and F(ψ,ϕ)-contractions on M-metric spaces, Int. J. Nonlinear Anal. Appl. 8 (2017), 209-224.H. Monfared, M. Azhini and M. Asadi, A generalized contraction principle with control function on M-metric spaces, Nonlinear Functional Analysis and Appl. 22 (2017), 395-402.W. Onsod, P. Kumam and Y. J. Cho, Fixed points of α-θ-Geraghty type and θ-Geraghty graphic type contractions, Appl. Gen. Topol. 18 (2017), 153-171. https://doi.org/10.4995/agt.2017.6694N. Y. Özgür, N. Mlaiki, N. Taş and N. Souayah, A generalization of metrics spaces: rectangular M- metric spaces, Math. Sci. 12 (2018), 223-233. https://doi.org/10.1007/s40096-018-0262-4H. Piri and P. Kumam, Some fixed point theorems concerning F-contraction in complete metric spaces, Fixed Point Theory Appl. 2014 (2014), 210. https://doi.org/10.1186/1687-1812-2014-210H. Piri, S. Rahrovi, H. Marasi and P. Kumam, F-contraction on asymmetric metric spaces, J. Math. Comput. Sci. 17 (2017), 32-40. https://doi.org/10.22436/jmcs.017.01.03S. Reich, Some remarks concerning contraction mappings, Canad. Math. Bull. 14 (1971), 121-124. https://doi.org/10.4153/CMB-1971-024-9H. Sahin, A new type of F-contraction and their best proximity point results with homotopy application, Acta Applicandae Mathematicae 179 (2022), 1-15. https://doi.org/10.1007/s10440-022-00496-9H. Sahin, I. Altun and D. Turkoglu, Two fixed point results for multivalued F-contractions on M-metric spaces, Rev. R. Acad. Cienc. Exactas Fís. Nat. Ser. A Mat. RACSAM 113 (2019), 1839-1849. https://doi.org/10.1007/s13398-018-0585-xS. Shukla, Partial rectangular metric spaces and fixed point theorems, Sci. 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    Analysis of nighttime streamer corona discharges in storm clouds with ASIM data

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    Tesis del Departamento de Sistema Solar del Instituto de Astrofísica de Andalucía. Leída en el Salón de Actos del IAA el 17 de marzo del 2023, a las 12:00 h .[EN] The main objective of this doctoral thesis is to exhaustively study the corona-type electrical discharges that take place in storm clouds. Corona discharges are characterized, among other things, by transient optical emissions in the near ultraviolet and visible blue range (280 - 450 nm). This is why they have been called Blue LUminous Events (BLUEs). This thesis presents the first worldwide nighttime climatology of corona discharges in storm clouds by combining two years of BLUEs data recorded by MMIA instrument of ASIM on-board the ISS (Neubert et al., 2019). This doctoral thesis focuses on investigating the physics of BLUEs, with the aim of un- derstanding their nature and determining the mechanisms that produce them. Addition- ally, the thesis addresses the detailed analysis of the geographic and seasonal distribution of BLUEs is addressed from two years of unique data obtained by the Modular Multispec- tral Imaging Array (MMIA) of the European Space Agency’s (ESA) Atmosphere Space Interaction Monitor (ASIM) instrument that was launched into space on April 18, 2018 and has been operational at the International Space Station (ISS) since then. MMIA has three fast photometers (100 kHz) and two cameras. The photometers have interferential filters centered on the wavelengths 337.0 nm (with a width of 4 nm), 777.4 nm (with a width of 5 nm) and a wide filter between 180 nm and 230 nm. The two available cameras use filters centered at 337.0 nm and 777.4 nm with the same characteristics as the light meter filters. The doctoral thesis is presented as a collection of three scientific articles in which I am the first author. These articles have been published in high-impact journals in the field of atmospheric sciences (atmospheric electricity). The articles are preceded by a thesis index, a summary (in Spanish and English), an introduction, the motivation of the studies carried out, a brief description of the methodology that has been followed and a concise presentation of the BLUEs. In my first article (published in Journal of Geophysical Research - Atmospheres, 2020, and highlighted by the editor) the structure of the BLUEs is described based on the observations of a storm recorded by ASIM on May 14, 2019 over Indonesia. The events were observed using the 337.0 nm photometer, during periods of little or no concurrent activity in the photometer centered on the 777.4 nm band (which is typical for lightning optical emissions). Through radio measurements made from the ground, it was concludedthat 7 of the 10 cases analyzed corresponded to positive narrow bipolar events (NBE). NBEs are characterized by being very strong radio frequency (RF) pulses with three important features: (1) their very short duration (about 20 microseconds), (2) a bipolar appearance (very fast rise and fall of two radio pulses of positive and negative polarity or vice versa) of the waveform in the VLF / LF frequency range (10 - 400 kHz) and (3) followed by extremely powerful bursts of radiation. on VHF / HF (3 - 300 MHz). NBEs, when detected in the VLF/LF range, are typically ten times more intense than radio emissions in the high frequency (HF) range typically emitted by normal intracloud and/or intercloud lightning.. In addition, recent observations (2016 and 2017) suggest that NBEs are the result of very fast processes of electrical breakdown in air. Fast breakdown is associated to cold electrical discharges, that is, those that do not heat the surrounding air (unlike normal lightning) and in which the temperature of the ambient electrons reaches very high values of up to 80000 ◦C (about 7 eV) (electron volts). The fact that electrons have a small mass (2000 times lighter than the lightest atom) prevents them from heating the surrounding air. In this first work, a new and innovative method was developed to determine the height of BLUEs in storm clouds from the analysis of their optical signals. In particular, the method is based on fitting the 337.0 nm light curves captured by the MMIA 337.0 nm photometer to a model of light diffusion in storm clouds. The height obtained agrees well with measurements carried out with methods based on ground-based radio detection. The altitude at which these NBEs occur ranges between 8.5 km and 14 km. Obser- vations indicate that single-pulse blue flashes are caused by streamers (air plasma darts with strong head ionization) which, as discussed above, do not heat the air (they are cold discharges). The findings discussed in the first paper led us to conclude that positive NBEs are corona discharges made up of hundreds of millions of positive streamers (the head of the streamer carries positive electrical charge) that form in thunderclouds and that the BLUEs are the optical manifestation of the NBEs. My second article (published in Geophysical Research Letters, 2021), focuses on the global analysis of the blue pulses observed in storm clouds, focusing on studying the relationship of the BLUEs with lightning, both annually and seasonally. For this, a new algorithm has been developed and used to be able to filter the raw information from MMIA, and systematically obtain only the activity of BLUEs, excluding the rest of electrical interactions in storm clouds. The result of this comprehensive work is the first, and so far the only, nocturnal climatology of BLUEs (corona discharge activity in storm clouds) obtained from data from the ASIM MMIA instrument. Our research concluded that approximately 11 BLUEs occur globally every second at local midnight, and the average number of BLUEs on land/sea is 7 to 4. Geographically, the peak ofthe distribution of BLUEs is located in a region in northwestern Colombia. Three main zones of atmospheric electrical activity are shown in this distribution: America, Europe / Africa, and Asia / Australia. A zone of weaker BLUE electrical activity has also been found in the Pacific. My third paper (published in Journal of Geophysical Research - Atmospheres, 2022) delves into the results of the second, and focuses on distinguishing different types of blue pulses based on the goodness of their fit with the ”first hitting model” or FHM (model of diffusion of light in storm clouds) and in extracting its main characteristics such as optical power density (μW m−2) of the 337.0 nm pulse maximum, rise time of maximum, total duration, brightness, etc, based on the fit and raw data. In addition, we also found two types of global distributions of BLUEs, depending on whether an extra criteria is applied (or not) to the algorithm of the previous work (paper two) on the South Atlantic Magnetic Anomaly (SAA). This additional criteria is included because a clear oversensing of cosmic rays was observed with ASIM in the SAA region. The extra criteria aims to limit the number of cosmic rays detected by putting a limit on the duration of the events detected in the SAA. It is concluded that the real number of BLUEs would range between the two distributions found in this third work. The analysis of the characteristics of the BLUEs indicates that around 10% of the events are clearly BLUEs with a clear maximum. Most of them have a peak optical power density below 25 μW/m2, occur up to 4 km below the upper cloud boundary and are made up of hundreds of millions of streamers (up to 3 × 109).[ES] El objetivo de esta tesis doctoral es estudiar de forma exhaustiva las descargas el ́ectricas de tipo corona que tienen lugar en las nubes de tormenta. Las descargas corona se caracterizan, entre otras cosas, por emitir luz en el rango ultravioleta cercano y azul (280 - 450 nm). Es por esto por lo que se las ha llamado Blue LUminous Events (BLUEs). Esta tesis presenta la primera climatolog ́ıa nocturna de descargas de corona en las nubes de tormenta combinando dos a ̃nos de datos de BLUEs recogidos por el instrumento MMIA de ASIM a bordo de la ISS (Neubert et al., 2019). La tesis se centra en, por un lado, investigar la f ́ısica de los BLUEs, esto es, en descifrar su naturaleza y en determinar cu ́ales son los mecanismos que los producen. Por otra lado, se aborda el an ́alisis detallado de la distribuci ́on geogr ́afica y estacional de los BLUEs a partir de dos a ̃nos de datos obtenidos por el Modular Multispectral Imaging Array (MMIA) del instrumento Atmosphere Space Interaction Monitor (ASIM) de la Agencia Espacial Europea (ESA) que fue lanzado al espacio el 18 de abril de 2018 y que est ́a operativo en la Estaci ́on Espacial Internacional (ISS) desde entonces. MMIA est ́a formado por tres fot ́ometros r ́apidos (100 kHz) y dos c ́amaras. Los fot ́ometros disponen de filtros interferenciales centrados en las longitudes de onda 337.0 nm (con una anchura de banda de 4 nm), 777.4 nm (con una anchura de banda de 5 nm) y un filtro ancho entre 180 nm y 230 nm. Las dos c ́amaras disponibles usan filtros centrados en 337.0 nm y 777.4 nm con las mismas caracter ́ısticas que los filtros de los fot ́ometros. La tesis doctoral se presenta como una colecci ́on de tres art ́ıculos cient ́ıficos en los que soy primer autor. Estos art ́ıculos sobre electricidad atmosf ́erica han sido publicados en revistas de alto impacto en el campo de las ciencias atmosf ́ericas. Los art ́ıculos vienen precedidos por un ́ındice de la tesis, un resumen (en espa ̃nol e ingl ́es), una introducci ́on, la motivaci ́on de los estudios realizados, una breve descripci ́on de la metodolog ́ıa que se ha seguido y una descripci ́on concisa de los BLUEs. En mi primer art ́ıculo (publicado en Journal of Geophysical Research - Atmospheres, 2020, y destacado por su editor) se describe la estructura de los BLUEs apoy ́andose en las observaciones de una tormenta registrada por ASIM el 14 de Mayo de 2019 sobre Indonesia. Los eventos fueron observados con el fot ́ometro 337.0 nm, sin actividad con- currente, o despreciable en el fot ́ometro centrado en la banda 777.4 nm (emisiones t ́ıpicas de rayos). A trav ́es de mediciones de radio efectuadas desde el suelo, se concluy ́o que 7de los 10 casos analizados correspond ́ıan a eventos bipolares estrechos positivos o positive narrow bipolar events (NBE) en ingl ́es. Los NBEs se caracterizan por ser pulsos muy fuertes de radiofrecuencia (RF) con tres rasgos importantes: (1) su muy corta duraci ́on (apenas 20 microsegundos), (2) un aspecto bipolar (muy r ́apida subida y bajada de dos pulsos de radio de polaridad positiva y negativa o viceversa) de la forma de onda en el rango de frecuencias VLF / LF (10 - 400 kHz) y (3) por venir habitualmente seguidos de potent ́ısimos estallidos de radiaci ́on VHF / HF (3 - 300 MHz). Los NBE detectados en el rango VLF / LF son por lo general diez veces m ́as intensos que las emisiones de radio en el rango de alta frecuencia (HF) procedentes de rayos normales intranube o entre nubes. Adem ́as, observaciones recientes (2016 y 2017) parecen sugerir que los NBEs son el resultado de procesos muy r ́apidos de ruptura el ́ectrica del aire t ́ıpicos de descargas el ́ectricas fr ́ıas, esto es, aquellas que no calientan el aire circundante (al contrario que los rayos normales) y en las que la temperatura de los electrones ambientales alcanzan valores muy elevados de hasta 80000 ◦C (unos 7 eV [electr ́on voltios]). El hecho de que los electrones tengan una masa muy peque ̃na (2000 veces m ́as ligeros que el ́atomo m ́as liviano) impide que, a ́un siendo muy energ ́eticos, puedan calentar el aire circundante. En este primer trabajo se desarroll ́o un nuevo y novedoso m ́etodo para determinar la altura de los BLUEs en las nubes de tormenta a partir del an ́alisis de sus se ̃nales ́opticas. En particular, el m ́etodo se basa en ajustar las curvas de luz captadas por el fot ́ometro centrado en 337.0 nm de MMIA a un modelo de difusi ́on de luz en las nubes de tormenta. La altura obtenida concuerda bien con medidas realizadas con m ́etodos basados en radio detecci ́on. La altitud a la que ocurren estos NBEs se sit ́ua aproximadamente entre 8.5 y 14 km. Las observaciones indican que los flashes azules con un solo pulso son originados por streamers (dardos de plasma de aire con fuerte ionizaci ́on en la cabeza) que, como se ha mencionado, no calientan el aire, esto es, son descargas fr ́ıas, la luz emitida por streamers es pues la manifestaci ́on ́optica de dichos NBEs. Los hallazgos que se discuten en el primer trabajo nos llevaron a concluir que los NBEs positivos son descargas corona formadas por cientos de millones de streamers positivos (la cabeza del streamer transporta carga el ́ectrica positiva) que se forman en las nubes de tormenta y que los BLUEs son la manisfestaci ́on ́optica de dichos NBEs. Mi segundo art ́ıculo (publicado en Geophysical Research Letters, 2021), se centra en el an ́alisis a nivel global de los pulsos azules observados en las nubes de tormenta, de- teni ́endose en estudiar la relaci ́on de los BLUEs con los rayos, tanto anual como esta- cionalmente. Para ello se ha desarrollado y utilizado un novedoso algoritmo para poder filtrar la informaci ́on en bruto de MMIA, y obtener sistem ́aticamente s ́olo la actividadde BLUEs excluyendo el resto de interacciones el ́ectricas en las nubes de tormenta. El resultado de este completo trabajo es la primera, y hasta ahora la ́unica, climatolog ́ıa nocturna de BLUEs (coronas en nubes de tormenta) obtenida a partir de datos del instrumento MMIA de ASIM. En nuestra investigaci ́on se concluy ́o que, aproximada- mente, tienen lugar unos 11 BLUEs a nivel global cada segundo en la media noche local, y que el promedio de BLUEs en tierra / mar es de 7 a 4. Geogr ́aficamente, el pico de la distribuci ́on de BLUEs est ́a localizado en una regi ́on al noroeste de Colombia. En esta distribuci ́on se muestran tres zonas principales de actividad el ́ectrica atmosf ́erica: Am ́erica, Europa/ ́Africa, y Asia/Australia. Tambi ́en se ha encontrado una zona de ac- tividad el ́ectrica m ́as d ́ebil en el Pac ́ıfico. Mi tercer trabajo (publicado en Journal of Geophysical Research - Atmospheres, 2022) profundiza en los resultados del segundo, y se centra en distinguir distintos tipos de pulsos azules en funci ́on de la bondad de su ajuste con el ”first hitting model” ́o FHM (modelo de difusi ́on de luz en las nubes) y en obtener sus principales caracter ́ısticas tales como densidad de potencia ́optica (μW m−2) del m ́aximo del pulso 337.0 nm, tiempo de subida del m ́aximo, duraci ́on total, brillo, etc, con base al ajuste y a los datos en bruto. Adem ́as, tambi ́en encontramos dos tipos de distribuciones globales de BLUEs, dependiendo de si se aplica (o no) un criterio extra al algoritmo del anterior trabajo en la anomal ́ıa magn ́etica del Atlantico Sur (SAA). Este criterio adicional se incluye debido que se observ ́o una clara sobredetecci ́on de rayos c ́osmicos con ASIM en la zona de la SAA. El criterio extra pretende limitar el n ́umero de rayos c ́osmicos detectados poniendo un l ́ımite en la duraci ́on de los eventos detectados en la SAA. Se estima que la cifra real de BLUEs se hallar ́a entre las dos distribuciones encontradas en este ́ultimo trabajo. El an ́alisis de las caracter ́ısticas de los BLUEs nos indica que alrededor del 10% de los eventos son claramente BLUEs con un m ́aximo claro. La mayor ́ıa de ellos tiene una densidad de potencia ́optica por unidad de superficie de pico por debajo de 25 μW/m2, ocurren a una distancia de hasta 4 km por debajo del l ́ımite superior de la nube y est ́an formados por cientos de millones de streamers (hasta 3 × 109).This thesis was supported by the Spanish Ministry of Science and Innovation, Min- isterio de Ciencia e Innovaci ́on (AEI) under project ESP2017-86263-C4-4-R, PID2019- 109269RB-C43 and the FEDER program. I acknowledge a PhD research contract through the project ESP2017-86263-C4-4-R and I also acknowledge financial support from the State Agency for Research of the Spanish MCIU through the “Center of Excellence Severo Ochoa” award for the Instituto de Astrof ́ısica de Andaluc ́ıa (SEV-2017-0709).Peer reviewe
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