Geophysical Institute, University of Alaska, Fairbanks

GSE Forecasts
Geoeffectiveness of Solar Events

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3-Dimensional View of the Heliospheric Current Sheet

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VRML-enabled browser required. See below.

3-D Heliospheric Current Sheet

3-D Solar Source Surface Maps
at 2.5 Solar Radii

Click to see VRML version
Click on image to get the 3-D view

Check out the daily snapshots of the 3-D images

Note: Presently, the velocity and density links may bring up the magnetic field map instead. We are working on the problem.

Description:

The green surface is the Heliospheric Current Sheet (HCS).  Earth and its orbit are blue, Mars is red, Venus is yellow.   The Sun is either blue or red, depending upon whether you are in a toward or away sector (described in the next paragraph).  Use the VRML console to zoom, rotate, pan, etc.  Click on the Sun to see a close-up of the solar source surface.  Put the mouse on the green words (you can drag them to the side).  You can then turn off/on the data, the grid, equatorial plane, etc.  Click on prev/next to bring up an earlier/later day's HCS.

We generate 3-D displays of the HCS daily.  The HCS is a surface separating the sunward (toward) and anti-sunward (away) directed interplanetary magnetic field (IMF).  In the ecliptic plane, the boundary separating the toward and away directed IMF is called the sector boundary.  Geomagnetic storms often occur as sector boundary sweeps past the Earth.  The HCS is the three dimensional extension of sector boundaries.  Early researchers hypothesized the HCS would take the shape of a ballerina skirt.

We model the solar wind and IMF using the Hakamada-Akasofu-Fry (HAF) solar wind model.  We also provide real-time space weather forecasts as soon as possible following significant solar events.

Source surface maps:

Blue represents negative magnetic field (points toward the Sun).   Red represents areas of positive (or away) fields.  Click on the sphere to see the original source surface map.

We obtain daily solar source surface maps from the NOAA/SEC Rapid Prototyping Center (Arge and Pizzo, J. Geophys. Res., 105, pp. 10,465-10,479, 2000).  These maps provide the boundary conditions for HAF to compute the ambient, inhomogeneous background solar wind conditions.  We also compute source surface maps using Hakamada's technique (K. Hakamada, Solar Phys., 159, pp. 89-96, 1995).

You will need a VRML plug-in to view these displays

The Cosmo Player VRML plug-in works well with IE 6 and Netscape.  Download Cosmo Player. 

The Cortona plug-in may also work, but we have experienced a few glitches using the version 3 of this browser.  Download the latest version.

* Note: Thanks to Ed Hoch, GEDDS Project Manager, for computing the HCS and developing these displays.

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