apodman wrote:From the lack of meteors shown originating from far Southern declinations, I conclude that Japan is in the Northern hemisphere.
It's true enough, you can only record meteors that you can see <g>. I have the same issue recording meteors from Colorado:
That said, there is more meteor shower activity in the northern hemisphere- a temporary condition lasting a few centuries or longer and representing nothing more than a statistical artifact.
I wouldn't mind further explanation of the color/velocity scale and why different radiants show different characteristic velocities. Is it simply the vector sum of the earth's orbital velocity and the particles' orbital velocities? Or has the earth's velocity been subtracted out to show just the meteroid's orbital velocity around the sun?
Different radiants have different velocities because their parent debris is in different orbits. The colors represent geocentric velocities- the velocity with respect to the center of the Earth. That velocity is primarily determined by the vector sum of the Earth and particle orbital velocities. However, there is a component of the velocity resulting from gravitational attraction to the Earth. High velocity showers like the Leonids (LEO) are caused by debris in retrograde orbits.
Is the shown velocity the extrapolated original velocity or the observed velocity after atmospheric drag has come into play? Given observed velocity, how could extrapolation determine the original velocity?
Atmospheric drag is not included. When you measure a meteor's velocity, you extrapolate backwards to the initial velocity, called V
inf. I do that by looking at velocity versus time, and using a model that incorporates details of upper atmospheric density as a function of height, and also at ablation characteristics.
Can someone enlighten me about such terms as V_heliocentric (Vh), V_apparent (Va), and V_geocentric (Vg)? What is zenith attraction?
Heliocentric velocity is the velocity with respect to the Sun. This is used in determining the parent body orbit. Geocentric velocity is the velocity with respect to the center of the Earth. Apparent velocity can mean different things; with meteors, I use it to mean with respect to the observer, and it therefore includes velocity components from the rotation of the Earth. Zenith attraction refers to the fact that a meteoroid's path is deflected towards the center of the Earth by gravity as it gets nearer our planet. This has the effect of making the radiant appear closer to the zenith (higher) than it actually is.
All of this stuff matters when you analyze a meteor. Using data from two or more stations, you can determine the atmospheric path and velocity. You extrapolate the speed back to get the initial value, and the path back as well, compensating for zenith attraction. You end up with a state vector (3 values for position, 3 values for velocity). That vector describes an
apparent state. This gets decomposed into a
geocentric state by compensating for the observer's position and rotational velocity. Then this gets decomposed into a
heliocentric state by removing the orbital effects of the Earth. The orbital elements of the meteoroid can now be calculated. It's a bit of a grunge... thank goodness for computers!