1,721,029 research outputs found
Color Figures for: SPACE WEATHER RESEARCH AND FORECAST IN USA article
No full textColor figures for article in Conference Proceedings of XX annual conference on solar and solar-terrestrial physics held at the Main (Pulkovo) Astronomical Observatory, 10-14 Oct. 2016, Author: A.A. Pevtso
G-band movie of solar granulation
No full textG-band movie of solar granulation taken at Dunn Solar Telescope (DST), National Solar Observatory at Sacramento Pea
Synoptic maps of vector magnetic field (CR2109-2131)
No full textFirst ever synoptic maps of photospheric vector magnetic field were developed at NSO. These maps, based on full disk vector magnetograms from SOLIS/VSM give a snapshot of vector magnetic field components on the sun during Carrington rotations 2109-2131
X-RAY RADIANCE AND MAGNETIC FLUX
No full textSoft X-ray and magnetic field observations of the Sun (quiet Sun, X-ray bright points, active regions, and integrated solar disk) and active stars (dwarf and pre–main-sequence) that were used in Figure 1 in Pevtsov et al (2003) in their study of X-ray spectral radiance LX vs. total unsigned magnetic flux for solar and stellar objects
Synoptic maps for Lagrangian L1 and L5 modeling
No full textTwo sets of Near-Real-Time (NRT) synoptic maps from SOLIS/VSM. One is a complete (used for modeling "true" distribution of magnetic field on the Sun, and another with two isolated bipolar active regions removed to model the observations from L1 point
Synoptic maps of vector magnetic field (CR2109-2131)
No full textFirst ever synoptic maps of photospheric vector magnetic field were developed at NSO. These maps, based on full disk vector magnetograms from SOLIS/VSM give a snapshot of vector magnetic field components on the sun during Carrington rotations 2109-2131
G-band movie of solar granulation
No full textG-band movie of solar granulation taken at Dunn Solar Telescope (DST), National Solar Observatory at Sacramento Pea
X-RAY RADIANCE AND MAGNETIC FLUX
No full textSoft X-ray and magnetic field observations of the Sun (quiet Sun, X-ray bright points, active regions, and integrated solar disk) and active stars (dwarf and pre–main-sequence) that were used in Figure 1 in Pevtsov et al (2003) in their study of X-ray spectral radiance LX vs. total unsigned magnetic flux for solar and stellar objects
Synoptic Maps of Uncertainties
No full textSample of synoptic magnetic field and corresponding uncertainty maps for Carrington rotations 2093 and 213
Synoptic maps from different Lagrangian points
No full textThe synoptic maps of pseudo-radial magnetic field as if there observed from Lagrangian points L1, L1+L5, L1+L5+l4, L1+L5+L4+L3, L1+SolO out of ecliptic location, and true magnetic field used for creating these synoptic maps. The data are based on a realistic model of solar magnetic field over one cycle
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