Stanford Helioseismology Archive - prog:moth

Magneto-Optical Two-Height Instrument

The data in this program are derived from observations made with the MOTH (Magneto-Optical Two-Height) Instrument at the Jeffreys Solar Observatory at the South Pole.

***** RESTRICTIONS ON USE OF THESE DATA *****

Include any guidelines for data users, including requested acknowledgments in published results making use of the data **************************************************

For further information, please contact Wolfgang Finsterle, WFinsterle @ spd.aas.org

Available Data Series

Calibrated images are organized by the observable (Doppler or Intensity) and line (Sodium-D or Potassium-D). Each hourly data set contains a nominal 360 images at a cadence of 10 seconds.


This page last revised Wednesday, 19-Jun-2013 11:48:33 PDT.
Please address page comments and questions to Rick Bogart


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