Realtime Monitoring - Magnetosphere, Solar Wind, Corona

STEREO consists of two space-based observatories - one ahead of Earth in its orbit, the other trailing behind. With this new pair of viewpoints, scientists will be able to see the structure and evolution of solar storms as they blast from the Sun and move out through space.

• http://stereo.gsfc.nasa.gov/

• http://stereo-ssc.nascom.nasa.gov/beacon/beacon_secchi.shtml
• http://stereo-ssc.nascom.nasa.gov/browse/

The images above are shown in the order of the relative positions of the three viewpoints, Behind, Earth, and Ahead. For the Heliospheric Imager (HI) images below, the order is reversed to reflect the fact that the HI Ahead telescopes look to the left of the Sun, and those on Behind look to the right. Also, the HI images are not rotated to put solar north up.

• http://sohowww.nascom.nasa.gov/data/realtime-images.html SOHO

Farside

• http://gong.nso.edu/data/farside/

• http://stereo-ssc.nascom.nasa.gov/where.shtml

This figure plots the current positions of the STEREO Ahead (red) and Behind (blue) spacecraft relative to the Sun (yellow) and Earth (green). The dotted lines show the angular displacement from the Sun. Units are in A.U.

When the two spacecraft are close to Earth, an expanded view of the region around Earth will appear on the right, in the same orientation as the Sun-centered view.

• http://www2.nict.go.jp/y/y223/simulation/realtime/

Earthquake

• CORONA, Proton Activities Chart

• HAARP
• magnetometer
• riometer

WINDMI results: blue: Rectified , red: Siscoe , green: Newell driver

Driving voltages for WINDMI (blue: Rectified, red: Siscoe, green: Newell):

State variables within WINDMI (set a):

State variables within WINDMI (set b):

• http://ccmc.gsfc.nasa.gov/
• http://ccmc.gsfc.nasa.gov/realtime.php
• http://iswa.gsfc.nasa.gov:8080/IswaSystemWebApp/
• http://ccmc.gsfc.nasa.gov/awareness/
• http://ccmc.gsfc.nasa.gov/awareness/directory.html

Solar

• EIT 171 A
• EIT 195 A
• EIT 284 A
• EIT 304 A
• Stereo Ahead
• Stereo Behind
• Goes X-Ray
• Goes proton and electron flux
• Solar Photospheric Magnetogram with FL tracing (Kitt Peak, WSA, ENLIL)
• Solar Photospheric Magnetogram with FL tracing (Gong, WSA, ENLIL)
• Solar Coronal Magnetic Field (PFSS, J. Luhmann et al.)

Heliosphere

• SOHO LASCO C2
• SOHO LASCO C3
• SOHO RD
• Stereo Ahead coronograph
• Stereo Behind coronograph
• SOHO/COSTEP real-time proton flux
• SOHO/COSTEP proton flux forecast
• ACE ion density and magnetic field
• ACE and STEREO-B (Time shifted to predict conditions at ACE)
• Stereo Beacon
• Stereo Beacon Ahead
• Stereo Beacon Behind
• Enlil ion density and polarity time series
• Synoptic Map - Ion density (Heliospheric Tomography, B. Jackson, P. Hick) Click image for movie
• Synoptic Map - Velocity (Heliospheric Tomography, B. Jackson, P. Hick) Click image for movie
• ACE ion density
• SW velocity
• Density and magnetic field polarity in ecliptic plane (Enlil, Odstrcil, NOAA)

Magnetosphere

• Kp indices
• Radiation Belt electron fluxes 10 keV
• Radiation Belt electron fluxes 20 keV
• Radiation Belt electron fluxes 50 keV
• Radiation Belt electron fluxes 100 keV
• Radiation Belt electron fluxes 200 keV
• Radiation Belt electron fluxes 400 keV
• Radiation Belt electron fluxes 1000 keV
• Radiation Belt electron fluxes 2000 keV
• Radiation Belt electron fluxes 4000 keV
• Plasma density, velocity and magnetic field - north-south cut (SWMF, T. Gombosi et al.)
• Plasma density, velocity and magnetic field - equatorial cut (SWMF, T. Gombosi et al.)
• Electrons at 1.7 KeV Particle Fluxes in Inner Magnetosphere (Fok Ring Current, M. Fok)
• Electrons at 22.5 KeV Particle Fluxes in Inner Magnetosphere (Fok Ring Current, M. Fok)
• Electrons at 300 KeV Particle Fluxes in Inner Magnetosphere (Fok Ring Current, M. Fok)
• Protons at 1.7 KeV Particle Fluxes in Inner Magnetosphere (Fok Ring Current, M. Fok)
• Protons at 22.5 KeV Particle Fluxes in Inner Magnetosphere (Fok Ring Current, M. Fok)
• Protons at 300 KeV Particle Fluxes in Inner Magnetosphere (Fok Ring Current, M. Fok)
• Current Magnetopause Position (SWMF, T. Gombosi et al.) Click on image for 24-hour history movie
• 3-day history of magnetopause standoff (SWMF, T. Gombosi et al.)
• Magnetic field at GOES-11 and GOES-12 (SWMF, T. Gombosi et al.)
• History plot of Dst from SWMF model (SWMF, T. Gombosi et al.)

Ionosphere

• Ionospheric High Frequency Vertical Signal Loss, 2.5 MHz Absorbtion (AbbyNormal, J. V. Eccles et al.)
• Ionospheric High Frequency Vertical Signal Loss, 5.0 MHz Absorbtion (AbbyNormal, J. V. Eccles et al.)
• Ionospheric High Frequency Vertical Signal Loss, 10.0 MHz Absorbtion (AbbyNormal, J. V. Eccles et al.)
• Ionospheric High Frequency Vertical Signal Loss, 20.0 MHz Absorbtion (AbbyNormal, J. V. Eccles et al.)
• Ionospheric potential with polar cap (SWMF, T. Gombosi et al.) Click image for movie
• Ionospheric field-aligned currents and polar cap (SWMF, T. Gombosi et al.)
• Geomagnetically induced electric fields - EX (A. Pulkkinen)
• Geomagnetically induced electric fields - EY (A. Pulkkinen)
• 7-day history of cross cap ionospheric potential difference (SWMF, T. Gombosi et al.)
• Ionospheric electric potential (Weimer 2005, D. Weimer)

Planetary Space Weather

• Earth - Solar Photospheric Magnetogram and Derived Coronal Holes (Gong, WSA, ENLIL)
• Mars - Solar Photospheric Magnetogram and Derived Coronal Holes (Gong, WSA, ENLIL)
• Mercury - Solar Photospheric Magnetogram and Derived Coronal Holes (Gong, WSA, ENLIL)
• Venus - Solar Photospheric Magnetogram and Derived Coronal Holes (Gong, WSA, ENLIL)
• ENLIL nowcast for solar wind conditions at Mercury.
• ENLIL nowcast for solar wind conditions at Venus.
• ENLIL nowcast for solar wind conditions at Mars.
• ENLIL nowcast for solar wind conditions at Earth.