University of Birmingham eData Repository (UBIRA E-Data)
Not a member yet
663 research outputs found
Sort by
An understanding of ‘strengths’ and ‘Strengths based approach’ within older people from ethnic minorities in the UK. A Qualitative Systematic Review
Full text linkPrisma Checklist and Prisma Abstract checklis
Research data supporting "Peer support intervention (ABA-feed) for improving breastfeeding: UK based, multicentre, parallel group, randomised controlled trial"
No full textResearch data for "Peer support intervention (ABA-feed) for improving
breastfeeding: UK based, multicentre, parallel group,
randomised controlled trial
Research data supporting the Thesis "A new geophysical survey across the Rockall Plateau passive margin; insights into the relationship between the North Atlantic Igneous Province and the Paleocene-Eocene Thermal Maximum"
No full textResearch data supporting the Thesis "A new geophysical survey across the Rockall Plateau passive margin; insights into the relationship between the North Atlantic Igneous Province and the Paleocene-Eocene Thermal Maximum
The feature-extraction and sequence-construction code
No full text1- user_id (account id for bot )
2- created_at (post timestamps)
3- action (Retweeting , Tweeting or Repleying)
4- is_url (Yes or No)
5- is_media (Photo , Video, No_Media)
6- is_emoji (Yes or No)
7- is_hash (Yes or No)
8- Text (Duplicated , Not-Duplicated or Empty)
9- Sentiment (Positive , Negative or Neutral )
10- G (First Generation, Second First Generation or Third First Generation)
11- letter_sequence ( group of 7 letters reprents the the encoded values of these features for one post of the bot )
The values of each features encoded into letter based on the following:
action = ("Tweeting" = "T", "Replying" = "Y", "Retweeting" = "R"),
is_url = ("YES" = "U", "NO" = "X"),
Sentiment = ("Positive" = "P", "Negative" = "N", "Neutral" = "L"),
is_media = ("Photo" = "I", "Video" = "V", "No_Media" = "M"),
Text = ("Duplicated" = "D", "Not-Duplicated" = "Q", "Empty" = "E"),
is_hash = ("YES" = "H", "NO" = "Z"),
is_emoji = ("YES" = "J", "NO" = "K"
Raw data for the article, "Uniaxial-Stress-Induced Magnetic Transitions in the Triangular-Lattice Antiferromagnet PdCrO2"
No full textThese are data files supporting a published article. For the X-ray diffraction data, the filename format is:
01_[run number]_V[V1]_[V2]_[h],[k],[l].cbf
The obverse peaks – the ones used to obtain the lattice constants and bond angles – are:
(2,0,-4) (run 2); (3,-2,-7) (run 3); (2,0,2) (run 4); (3,-2,-1) (run 5); (2,-2,-5) (run 8); (2,-2,-2) (run 10); (0,-1,1) (run 12); (0,-1,-2) (run 14); (-2,0,1) (run 17); (-2,0,4) (run 19); (-1,-2,-2) (run 21
Experimental Investigation of a Cryogenic-Enhanced ORC for Battery and Fuel-Cell Waste-Heat Recovery in Marine Hybrid Propulsion
No full textPaper Lin
Research data supporting "Gold(I) Dimers with Hemilabile Azophosphine Ligands in Catalysis"
No full textNMR, Mass spec, IR, UV-vis and computational data collected for the publication "Gold(I) Dimers with Hemilabile Azophosphine Ligands in Catalysis
Phases of interacting bosons in a hybrid Harper-Hofstadter system with a synthetic dimension of harmonic trap states: Data store
No full textData and code associated with research associated with pre-print paper titled "Phases of interacting bosons in a hybrid Harper-Hofstadter system with a system with a synthetic dimension of harmonic trap states
The seismic diversity of four successive solar cycle minima as observed by the Birmingham Solar-Oscillations Network (BiSON)
No full textWe have used data collected by the Birmingham Solar-Oscillations Network (BiSON) to perform a helioseismic diagnosis of changes to the Sun’s internal structure between four successive solar cycle minima, beginning with the minimum at the end of cycle 21 and ending with the recent minimum at the beginning of cycle 25. The unique duration of the BiSON data base makes such a study possible. We used the low-degree BiSON p-mode frequencies to constrain structural changes between minima in the layers above . We accomplished this by examining variations in the He ii ionization zone signature; and by inverting the frequency differences to infer changes in the sound speed. Additionally, we employed frequency differences between various solar models that had subtle modifications to their internal structures to facilitate analysis of the observations. We find evidence for small, but marginally significant, changes in structure between different minima. The He ii signature was larger, and the sound speed in the range to was slightly higher, during the cycle 23/24 minimum, than during the other minima. The cycle 23/24 minimum was the deepest, as measured by proxies of global solar activity. These findings are consistent with magnetic flux levels having been lower in this minimum than the others, resulting in a higher gas pressure, higher temperatures, and higher sound speed. Our results demonstrate the potential of using asteroseismic data to perform similar analyses on other solar-type stars.
The files contain frequency sets for each cycle minimum period, after weeding.
Columns are: (1) angular degree, l (2) overtone number n (3) frequency (uHz) (4) error (uHz)
Airgradient data from 6 sites in Kampala, Uganda
No full textAirgradient data from 6 sites in Kampala, Ugand
Data sources:
Access Repository Dashboard
Do you manage Open Research Online? Become a CORE Member to access insider analytics, issue reports and manage access to outputs from your repository in the CORE Repository Dashboard! 👇