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SDO, SID Monitors, and IHY

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One part of the ionospheric response to solar flares ... The inset graph shows my results compared with the satellite GOES-6. During the ... – PowerPoint PPT presentation

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Title: SDO, SID Monitors, and IHY


1
SDO, SID Monitors, and IHY
  • Dean Pesnell

2
What is a Sudden Ionospheric Disturbance?
Ionizing
Dissociating
  • One part of the ionospheric response to solar
    flares
  • X-rays and UV photons ionize the D-region (60-100
    km), increasing Ne
  • During a flare it is the increase in X-rays with
    ? lt 8 Å that cause the effects called SID

The atmosphere absorbs all radiation with ? lt 250
nm, with each wavelength being absorbed at a
different altitude.
3
What is a Sudden Ionospheric Disturbance?
  • VLF waves (3-30 kHz, ? 10-100 km) are reflected
    by the increased electron density
  • If you monitor a remote VLF station you can see
    the enhancements between you and the station

4
SID Monitor of Gote Flodqvist in Farste, Sweden
The inset graph shows my results compared with
the satellite GOES-6. During the meridian passage
of the Sun (and summertime) the sensitivity of
the system can be as good as C-level flares. The
transmitter location is Rugby, UK. It transmits
continuously at 60 kHz. One use of SID monitors
is to fill the gaps in the data of the
GOES-system. This satellite is in eclipse from
8-9 UTC.
5
Most VLF stations are in the Northern Hemisphere
All information courtesy of Bill Hopkins,
Technical Representative for Pacific-Sierra
Research Corp. Updated by Michael Hill Last
updated 06/20/04
6
SIDs, Standford, and SDO
  • Solar group at Stanford includes the PI for HMI,
    the helioseismic instrument on SDO
  • Same group has proposed to run 15-30 SID
    monitoring stations around the Earth
  • Need the equipment for each station
  • Have an expert on VLF waves at Sanford

7
SIDs and Education
  • Simple equipment
  • Intel-based Computer (serial-port compatible)
  • Receiver
  • Antenna
  • Communications (Internet or mail)
  • Skills Taught
  • Construction (build and align antenna)
  • Data capture
  • Data analysis
  • Cooperation with other schools

8
SIDs and Education
  • SIDs are a day-time phenomenon
  • Shows the effects of solar flares
  • Other areas of research
  • Build receiver for SIDs
  • Build receiver for whistlers (nighttime activity)
  • Build whistler spectrograph
  • VLF and the magnetosphere
  • VLF and lightning
  • Chemistry during recovery
  • Similar research was part of IGY
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