Solar gravity modes from ACRIM-SWM irradiance data

Details Solar gravity modes from ACRIM-SWM irradiance data Solar gravity modes from ACRIM-SWM irradiance data

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984sses.nasa..183f&link_type=abstract

In JPL Solar Seismology from Space. p 183-193 (SEE N85-25060 14-92)

Physics

9

Irradiation, Power Spectra, Radiometers, Solar Gravitation, Solar Maximum Mission, Solar Oscillations, Frequency Ranges, Statistical Analysis

Scientific paper

The record of 280 days of continuous data of the ACRIM radiometer on board the Solar Maximum Mission satellite is analysed in the frequency range from 10 to 80 μHz. Gravity modes of degree one and two with orders from about 10 to several hundreds can be localized. A statistical method to determine the fundamental period T0 and the rate of rotation νR as seen by rotational splitting is described and the results for 33.5 < T0 < 45.5 minutes and 0.4 < νR < 2.0 μHz presented. They indicate a rather high T0 and it cannot be excluded that it is above the upper limit analysed.

Affiliated with

Also associated with

No associations

Rating

Solar gravity modes from ACRIM-SWM irradiance data does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Solar gravity modes from ACRIM-SWM irradiance data, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar gravity modes from ACRIM-SWM irradiance data will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-739804