Hawkeye cusp boundary crossings select and plot

Show entries that match the following criteria:

Time span: (yyyy/mm/dd hh:mm:ss)

Start:

Stop:

Solar wind pressure: Low: High:nPa
Solar wind speed: Low: High:km/s
Solar wind density: Low: High:#/cc
Solar wind temperature: Low: High:eV (=11,605K)

Interplanetary magnetic field:

|B|: Low: High: nT

Phi: Low: High: degrees (azimuthal)

Theta: Low: High: degrees (latitude)

Dipole tilt: Low: High:

Geomagnetic indices:
Kp index: Low: High: (e.g, 2, 3-, 4+, etc.)
Dst index: Low: High:

Region specific:(by Tim Eastman)
Cusp type A - Magnetosheath to Magnetosphere
Cusp type B - Magnetosphere to Magnetosphere
Cusp type C - Magnetosphere to Magnetosheath
Cusp type D - Magnetosheath to Magnetosheath
Entry layer
Plasma mantle
Magnetopause
No boundary layer at magnetopause

Other boundary layer classifications

Coordinate used to show components (if applicable)?
Geocentric Solar Magnetic (GSM) Solar Magnetic (SM) Show both

Creators of the Hawkeye Boundary Layer Listing:
Tim Eastman
Plasmas International
Silver Spring, MD
(301) 587-0894
plasmas@smart.net plasmas@bellaltantic.net

Scott Boardsen
Raytheon ITSS Corporation
Greenbelt, MD 20771
(301) 286-0837
boardsen@ndadsb.gsfc.nasa.gov

Curator of the database and interface:
Howard Leckner
QSS, Greenbelt, Maryland
(301)286-9270
leckner@mail630.gsfc.nasa.gov

Responsible government official:
Shing Fung
Code 632, NASA/Goddard Space Flight Center
Greenbelt, MD 20771
(301) 286-6301
fung@ndadsb.gsfc.nasa.gov