Meteor.cpp   Meteor.cpp 
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* as published by the Free Software Foundation; either version 2 * as published by the Free Software Foundation; either version 2
* of the License, or (at your option) any later version. * of the License, or (at your option) any later version.
* *
* This program is distributed in the hope that it will be useful, * This program is distributed in the hope that it will be useful,
* but WITHOUT ANY WARRANTY; without even the implied warranty of * but WITHOUT ANY WARRANTY; without even the implied warranty of
* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
* GNU General Public License for more details. * GNU General Public License for more details.
* *
* You should have received a copy of the GNU General Public License * You should have received a copy of the GNU General Public License
* along with this program; if not, write to the Free Software * along with this program; if not, write to the Free Software
* Foundation, Inc., 59 Temple Place - Suite 330, Boston, MA 02111-1307, U SA. * Foundation, Inc., 51 Franklin Street, Suite 500, Boston, MA 02110-1335, USA.
*/ */
// This is an ad hoc meteor model // This is an ad hoc meteor model
// Could use a simple ablation physics model in the future // Could use a simple ablation physics model in the future
/* /*
NOTE: Here the radiant is always along the ecliptic at the apex of the Eart h's way. NOTE: Here the radiant is always along the ecliptic at the apex of the Eart h's way.
In reality, individual meteor streams have varying velocity vectors and the refore radiants In reality, individual meteor streams have varying velocity vectors and the refore radiants
which are generally not at the apex of the Earth's way, such as the Perseid s shower. which are generally not at the apex of the Earth's way, such as the Perseid s shower.
*/ */
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