Results 41 to 50 of about 41,536 (207)

Thermal Diagnostics with the Atmospheric Imaging Assembly onboard the Solar Dynamics Observatory: A Validated Method for Differential Emission Measure Inversions

, 2015
We present a new method for performing differential emission measure (DEM) inversions on narrow-band EUV images from the Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO). The method yields positive definite DEM solutions by
Boerner, P., Chen, F., Cheung, Mark C. M., Malanushenko, A., Peter, H., Schrijver, C. J., Testa, P.   +6 more
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Nonlinear Fast Magnetosonic Waves in Solar Prominence Pillars

The Astrophysical Journal, 2023
We investigate the properties of nonlinear fast magnetosonic (NFM) waves in a solar prominence, motivated by recent high-resolution and high-cadence Hinode/Solar Optical Telescope (SOT) observations of small-scale oscillations in a prominence pillar.
Leon Ofman, Therese A. Kucera, C. Richard DeVore   +2 more
doaj   +1 more source

The X-ray cycle in the solar-type star HD 81809

, 2008
(abridged) Our long-term XMM-Newton program of long-term monitoring of a solar-like star with a well-studied chromospheric cycle, HD 81809 aims to study whether an X-ray cycle is present, along with studying its characteristics and its relation to the ...
Baliunas, F. Favata, Favata, G. Micela, Hempelmann, Hempelmann, Hempelmann, J. H. M. M. Schmitt, J. Hall, Judge, Orlando, Orlando, Orlando, Peres, Pourbaix, Robrade, S. Orlando, S. Sciortino, Schmitt, Soderblom, Takeda, Tsuneta   +21 more
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The Absolute Abundance of Iron in the Solar Corona [PDF]

, 2000
We present a measurement of the abundance of Fe relative to H in the solar corona using a technique which differs from previous spectroscopic and solar wind measurements.
Arnaud M., Fludra A., J. W. Brosius, M. R. Kundu, Mewe R., R. J. Thomas, S. M. White, Veck N. J.   +7 more
core   +3 more sources

Soft X-ray telescope (SXRT) [PDF]

The soft X-ray telescope (SXRT) will provide direct images of the solar corona with spatial resolution of about 1 arcsecond. These images will show the global structure of the corona, the location and area of coronal holes, and the presence of even the ...
Moore, R.
core   +4 more sources

Exploring the Origin of Solar Energetic Electrons. I. Constraining the Properties of the Acceleration Region Plasma Environment

The Astrophysical Journal, 2023
Solar flare electron acceleration is an efficient process, but its properties (mechanism, location) are not well constrained. Via hard X-ray (HXR) emission, we routinely observe energetic electrons at the Sun, and sometimes we detect energetic electrons ...
Ross Pallister, Natasha L. S. Jeffrey
doaj   +1 more source

Variability of Solar Five-Minute Oscillations in the Corona as Observed by the Extreme Ultraviolet Spectrophotometer (ESP) on the Solar Dynamics Observatory Extreme Ultraviolet Variability Experiment (SDO/EVE)

, 2012
Solar five-minute oscillations have been detected in the power spectra of two six-day time intervals from soft X-ray measurements of the Sun observed as a star using the Extreme Ultraviolet Spectrophotometer (ESP) onboard the Solar Dynamics Observatory ...
Didkovsky, Leonid, Judge, Darrell, Kosovichev, Alexander, Wieman, Seth, Woods, Tom   +4 more
core   +1 more source

Solar Stereoscopy and Tomography

Living Reviews in Solar Physics, 2011
We review stereoscopic and tomographic methods used in the solar corona, including ground-based and space-based measurements, using solar rotation or multiple spacecraft vantage points, in particular from the STEREO mission during 2007--2010 ...
Markus J. Aschwanden
doaj  

On the Origin of the Dominant Waves in the Extended Solar Corona

The Astrophysical Journal
The extended solar corona at 10–30 solar radii is essentially devoid of all waves below 100 kHz other than triggered ion acoustic waves (TIAWs), which consist of a low-frequency (LF) electromagnetic wave at a frequency of a few Hz coupled to one or more ...
F. S. Mozer, O. V. Agapitov, O. Romeo, V. Roytershteyn, A. Voshchepynets   +4 more
doaj   +1 more source

New views on the emission and structure of the solar transition region

, 2010
The Sun is the only star that we can spatially resolve and it can be regarded as a fundamental plasma laboratory of astrophysics. The solar transition region (TR), the layer between the solar chromosphere and corona, plays an important role in solar wind
Aiouaz, Aiouaz, Athay, Athay, Axford, Bartoe, Bartoe, Bartoe, Basri, Bocchialini, Bohlin, Bonnet, Brekke, Brosius, Brosius, Brosius, Brown, Brueckner, Brueckner, Brueckner, Brynildsen, Büchner, Büchner, Chae, Chae, Chae, Chen, Chen, Chen, Chuanyi Tu, Culhane, Curdt, Curdt, Curdt, Curdt, Curdt, Curdt, Dammasch, Dammasch, De Pontieu, Del Zanna, Dere, Dere, Dere, Doschek, Doschek, Doschek, Dowdy, Doyle, Doyle, Doyle, Doyle, Eckart Marsch, Evershed, Evershed, Falconer, Fang, Feldman, Feldman, Feldman, Fontenla, Fontenla, Foukal, Foukal, Foukal, Gabriel, Golub, Gontikakis, Gouttebroze, Gouttebroze, Griffiths, Gunár, Guo, Habbal, Hansteen, Hansteen, Harra, Harrison, Harrison, Hassler, He, He, He, Heinzel, Hui Tian, Hénoux, Ichimoto, Imada, Innes, Innes, Jiansen He, Jin, Jordan, Katsukawa, Kneer, Lemaire, Lemaire, Lemaire, Li, Liu, Longcope, Madjarska, Madjarska, Magara, Mariska, Mariska, Marsch, Marsch, Marsch, Marsch, Marsch, Marsch, McClymont, McIntosh, McIntosh, McIntosh, McIntosh, Metcalf, Nicolas, Nicolas, Parnell, Patsourakos, Peter, Peter, Peter, Peter, Peter, Popescu, Priest, Raju, Ravindra, Reeves, Sakao, Santos, Schmieder, Schrijver, Seehafer, Sheeley, Solanki, Stucki, Teriaca, Teriaca, Teriaca, Teriaca, Teriaca, Teriaca, Tian, Tian, Tian, Tian, Tian, Tian, Tian, Tian, Tian, Tian, Tian, Tian, Tu, Tu, Tu, Ugarte-Urra, Ugarte-Urra, Ugarte-Urra, Vernazza, Vernazza, Vial, Vial, Vial, Wang, Wang, Warren, Watanabe, Webb, Werner Curdt, Wiegelmann, Wiegelmann, Wiegelmann, Wilhelm, Wilhelm, Wilhelm, Wilhelm, Wilhelm, Xia, Xia, Xia, Xu, Zhang, Zhang, Zhang, Zhang, Zhang, Zhang   +192 more
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