New HMI Science Nuggets are available at
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#5 "Comparison of sunspot properties in cycle 24 and 23"
contributed by Reza Rezaei
We analyze umbral area, magnetic field, and umbral intensity of the
sunspots during the rising phase of cycle 24. We do not find a significant
variation in either sunspot physical properties or distribution of sunspot
umbral area from previous cycles.
We invite those who use HMI data for their research, or whose research is
closely related to HMI science objectives, to contribute to the HMI science
nuggets. -- SDO/HMI team
>
New HMI Science Nuggets are available at http://hmi.stanford.edu/hminuggets,
featuring the following topic
#6 "Fickle Fields: Are Transient Magnetic Reversals Real?" contributed by
Brian Harker
We present observations from SDO/HMI of a magnetic transient observed in
NOAA 11429 during the M7.9 flare on 13 March 2012. The observed transient
showed an impulsive rotation of the field vector in response to the
white-light flare.
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We invite those who use HMI data for their research, or whose research is
closely related to HMI science objectives, to contribute to the HMI science
nuggets. -- SDO/HMI team
New HMI Science Nuggets are available at http://hmi.stanford.edu/hminuggets,
featuring the following topic
#7 "Measuring the Solar Radius with HMI during the Venus Transit of 2012"
contributed by Sebastien Couvidat
The Venus transit of 2012 allowed us to measure the solar radius around
6173Å with HMI: we obtained a value of 959.58″ at 1 AU, with a systematic
uncertainty larger than 0.27″.
We invite those who use HMI data for their research, or whose research is
closely related to HMI science objectives, to contribute to the HMI science
nuggets. -- SDO/HMI team