Keywords: Solar Prominence (2)

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Halloween Solar Storms from SOHO-EIT, 304 Angstroms
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Halloween Solar Storms from SOHO-EIT, 304 Angstroms

This view from SOHO-EIT in the 304 Angstrom band, shows a group ... (more)

This view from SOHO-EIT in the 304 Angstrom band, shows a group of active regions rotating back into view. This movie is synchronized to play with animation IDs 2959 (http://svs.gsfc.nasa.gov-vis-a000000-a002900-a002959) and 2961 (http://svs.gsfc.nasa.gov-vis-a000000-a002900-a002961). One obvious difference is that solar flares are not as visible at this wavelength than at the 195 Angstrom band. The 304 Angstrom filter was not used as frequently as the 195 Angstrom filter, so this movie has more jumps in its time coverage. For more information on how X-ray solar flares are classified (B, C, M, X), visit (http://www.spaceweather.com-glossary-flareclasses.html). (less)

Subject:
Science and Technology
Material Type:
Other
Provider:
NASA
UCAR Staff
Provider Set:
NASA GSFC Scientific Visualization Studio
Scientific Visualization Studio
Author:
Carl Walz
Edward Stone
Thomas Zurbuchen
Tom Bridgman
2002 llaF ,gnivloS melborP gnireenignE dna sretupmoC ot noitcudortnI

2002 llaF ,gnivloS melborP gnireenignE dna sretupmoC ot noitcudortnI

.desu si egaugnal gnimmargorp avaJ ehT .gninnalp dna ,tnemeganam ,ecneics ,gnireenigne ni ... (more)

.desu si egaugnal gnimmargorp avaJ ehT .gninnalp dna ,tnemeganam ,ecneics ,gnireenigne ni smelborp gnivlos rof seuqinhcet gnipoleved no si sisahpmE .scipot decnavda detceles dna scihparg retupmoc ,gnihcraes dna gnitros ,serutcurts atad ,sdohtem laciremun ,secafretni resu lacihparg ,stpecnoc gnimmargorp revoc smelborp gnimmargorp ylkeeW .esruoc eht fo sucof eht si tnempoleved dna ngised erawtfos detneiro-tcejbO .snoitacilppa cifitneics dna gnireenigne rof sdohtem lanoitatupmoc dna tnempoleved erawtfos latnemadnuf stneserp esruoc sihT (less)