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Solar flare forecasting model supported with artificial neural network techniques
DOI: 10.1016/j.asr.2007.06.070 Bibcode: 2008AdSpR..42.1464W

Li, R.; Wang, H. N.; Cui, Y. M. +2 more

Nowadays operational models for solar activity forecasting are still based on the statistical relationship between solar activity and solar magnetic field evolution. In order to set up this relationship, many parameters have been proposed to be the measures. Conventional measures are based on the sunspot group classification which provides limited…

2008 Advances in Space Research
SOHO 49
Recent advances in observations and modeling of the solar ultraviolet and X-ray spectral irradiance
DOI: 10.1016/j.asr.2007.09.026 Bibcode: 2008AdSpR..42..895W

Woods, Thomas N.

There have been significant, recent advances in understanding the solar ultraviolet (UV) and X-ray spectral irradiance from several different satellite missions and from new efforts in modeling the variations of the solar spectral irradiance. The recent satellite missions with solar UV and X-ray spectral irradiance observations include the X-ray S…

2008 Advances in Space Research
SOHO 44
Helioseismology and the solar cycle
DOI: 10.1016/j.asr.2006.12.033 Bibcode: 2008AdSpR..41..846H

Howe, Rachel

Helioseismic measurements stretching back for about three decades have clearly shown that the acoustic modes are sensitive to solar-cycle changes. 2006 marks the first full 11-year cycle of continuous observations from the Global Oscillation Network Group (GONG), and 10 years of observations with the Michelson Doppler Imager (MDI) aboard the SOHO …

2008 Advances in Space Research
SOHO 22
Segmentation of extreme ultraviolet solar images via multichannel fuzzy clustering
DOI: 10.1016/j.asr.2007.10.021 Bibcode: 2008AdSpR..42..917B

Hochedez, Jean-François; Delouille, Véronique; Barra, Vincent

The study of the variability of the solar corona and the monitoring of its traditional regions (Coronal Holes, Quiet Sun and Active Regions) are of great importance in astrophysics as well as in view of the Space Weather and Space Climate applications. Here we propose a multichannel unsupervised spatially constrained fuzzy clustering algorithm tha…

2008 Advances in Space Research
SOHO 20
Variations of the solar acoustic high-degree mode frequencies over solar cycle 23
DOI: 10.1016/j.asr.2007.03.014 Bibcode: 2008AdSpR..41..861R

Schou, J.; Rabello-Soares, M. C.; Korzennik, Sylvain G.

Using full-disk observations obtained with the Michelson Doppler Imager (MDI) on board the Solar and Heliospheric Observatory (SOHO) spacecraft, we present variations of the solar acoustic mode frequencies caused by the solar activity cycle. High-degree (100 < ℓ < 900) solar acoustic modes were analyzed using global helioseismology analysis …

2008 Advances in Space Research
SOHO 16
Comparing proton fluxes of central meridian SEP events with those predicted by SOLPENCO
DOI: 10.1016/j.asr.2007.08.003 Bibcode: 2008AdSpR..42.1492A

Lario, D.; Aran, A.; Sanahuja, B.

We have developed an operational code, SOLPENCO, that can be used for space weather prediction schemes of solar energetic particle (SEP) events. SOLPENCO provides proton differential flux and cumulated fluence profiles from the onset of the event up to the arrival of the associated traveling interplanetary shock at the observer’s position (either …

2008 Advances in Space Research
SOHO 15
Tilts and polarity separation in the sunspot groups and active regions at the ascending and descending phases of the cycle 23
DOI: 10.1016/j.asr.2007.02.082 Bibcode: 2008AdSpR..41..881Z

Zharkova, V. V.; Zharkov, S. I.

The Solar Feature Catalogues for sunspots and active regions measured with SOHO/MDI instrument and Ca II K3 spectroheliograph of the Paris-Meudon Observatory are analyzed with the automated classification technique for sunspot groups and active region polarities. We report the first classification results for daily variations of tilt angles (norma…

2008 Advances in Space Research
SOHO 14
Probing solar and stellar interior dynamics and dynamo
DOI: 10.1016/j.asr.2007.05.023 Bibcode: 2008AdSpR..41..830K

Kosovichev, Alexander G.

Solar and stellar activity is a result of complex interaction between magnetic field, turbulent convection and differential rotation in a star’s interior. Magnetic field is believed to be generated by a dynamo process in the convection zone. It emerges on the surface forming sunspots and starspots. Localization of the magnetic spots and their evol…

2008 Advances in Space Research
SOHO 12
Multi-scale reconnections in a complex CME
DOI: 10.1016/j.asr.2007.04.065 Bibcode: 2008AdSpR..42..858V

Mandrini, C. H.; van Driel-Gesztelyi, L.; Culhane, J. L. +6 more

A series of three flares of GOES class M, M and C, and a CME were observed on 20 January 2004 occurring in close succession in NOAA 10540. Types II, III, and N radio bursts were associated. We use the combined observations from TRACE, EIT, Hα images from Kwasan Observatory, MDI magnetograms, GOES, and radio observations from Culgoora and Wind/ WAV…

2008 Advances in Space Research
SOHO 12
The dynamics of the solar radiative zone
DOI: 10.1016/j.asr.2007.03.057 Bibcode: 2008AdSpR..41..855T

Turck-Chièze, Sylvaine; Talon, Suzanne

The picture of the solar radiative zone is evolving quickly. This review is separated in two parts. We first recall how the two powerful probes of the solar interior, namely the neutrinos and helioseismology have scrutinized the microscopic properties of the solar radiative plasma. Recent observations stimulate today complementary activities beyon…

2008 Advances in Space Research
SOHO 9