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Flares From the Giant ar 9433 on 24 April 2001
DOI: 10.1023/A:1027336117718 Bibcode: 2003SoPh..217..173J

Uddin, Wahab; Chandra, Ramesh; Joshi, Anita

We present Hα CCD observations of three small-to-medium-size two-ribbon flares observed in the giant AR 9433 on 24 April 2001. Flare observations at other associated wavelengths (e.g., soft X-rays (SXR), hard X-rays (HXR), microwaves (MW)) obtained from archives are also presented and compared. We have tested the Neupert effect for the most energe…

2003 Solar Physics
SOHO 4
Periodicities Near 160 Minutes in Flare Occurrence
DOI: 10.1023/A:1025629526201 Bibcode: 2003SoPh..215..327B

Bai, Taeil

The 160.01-min periodicity was originally found from line-of-sight velocities of the photosphere, and Kotov and Tsap reported a detection of the same periodicity in flare occurrence times. Intrigued by this, I analyze occurrence times of flares of cycles 19-23 to investigate periodicities in the neighborhood of 160 min, cycle by cycle. The 160.01-…

2003 Solar Physics
SOHO 2
Acceleration Effects in MDI Magnetogram Data
DOI: 10.1023/A:1024270615207 Bibcode: 2003SoPh..214..227N

Norton, A.; Settele, A.

Acceleration effects are found in the Michelson Doppler Imager (MDI) magnetogram data because changes in the line profiles during the 30-s measurement are introduced by underlying p-mode velocity variations. This imparts an oscillatory component to the magnetic flux signal. Simulated profiles using Maltby M and Harvard Smithsonian Reference Atmosp…

2003 Solar Physics
SOHO 0