Northern-Taurids 2008: visual data quicklook

Introduction

This page shows automated results of the Northern-Taurids 2008, based on visual data entered through the IMO electronic report form. Send your feedback regarding this page to Geert Barentsen or visit the project pages. Note that these automated results may not be suitable for scientific use!

Immy Activity profile
Immy Observer statistics
Immy Data access

Page generated: 2008 December 9 at 2:27 UT.

Activity profile

ZHRmax = 8 based on 493 Northern-Taurids in 596 data intervals, assuming fixed population index r = 2.3 and zenith correction 1/sin(hR).

ZHR graph

Time (UT)SolarlonnINTnNTAZHR
2008-09-27 23:00185.0782992+-1
2008-09-29 22:48187.0357247+-1
2008-10-02 14:09189.6311371+-0
2008-10-04 06:53191.30312152+-0
2008-10-08 06:01195.21318192+-0
2008-10-11 02:29198.0312261+-0
2008-10-12 06:17199.177432+-1
2008-10-16 20:49203.7391001+-1
2008-10-19 07:48206.17833102+-1
2008-10-20 19:13207.64559312+-0
2008-10-22 02:07208.92526303+-1
2008-10-22 22:57209.78943303+-1
2008-10-23 05:02210.04258303+-1
2008-10-24 02:29210.93240302+-0
2008-10-25 15:48212.48217172+-0
2008-10-28 01:14214.87040152+-0
2008-10-31 02:54217.93815283+-1
2008-11-01 20:49219.68711334+-1
2008-11-02 17:43220.55815304+-1
2008-11-03 19:39221.6417318+-1
2008-11-05 05:40223.06216304+-1
2008-11-06 15:10224.4627185+-1
2008-11-08 18:37226.61312103+-1
2008-11-11 19:57229.6831784+-1
2008-11-17 00:08234.89350174+-1
2008-11-18 14:53236.521865+-2
2008-11-21 10:46239.376762+-1

For each estimation interval: time is the middle of the interval, nINT is the number of observing periods and nNTA is the number of Northern-Taurids involved. ZHR = (1 + sum nNTA) / sum(Teff/C) where Teff is the effective observing time and C is the total correction for limiting magnitude, clouds and zenith correction. The solar longitudes refer to equinox J2000.0.

Observer statistics

Data has been received from 49 observers in 20 countries. Thank you for your efforts!

Spatial distribution

Spatial distribution

Temporal distribution

Temporal distribution

Table of observers

ObserverCountryTeffnNTA
Salvador Aguirre Mexico 42.90h 31
Pierre Bader Germany 6.80h 7
Geoff Carstairs Australia 0.75h 0
Ameya Deshpande India 1.50h 2
Ameya Deshpande India 3.00h 3
Mayuresh Desai India 3.00h 5
Mayuresh Desai India 3.00h 4
Sietse Dijkstra Netherlands 17.31h 21
Todor Dimitrov Bulgaria 9.91h 10
Jaroslaw Dygos Poland 0.83h 1
Wei Ge China 0.67h 0
William Godley United States 7.84h 6
Mitja Govedic Slovenia 4.13h 18
Valentin Grigore Romania 4.86h 6
Wayne T. Hally United States 43.97h 34
Vilem Heblik Czech Republic 5.42h 10
Carl Hergenrother United States 1.54h 0
Kamil Hornoch Czech Republic 8.73h 17
Petr Horalek Czech Republic 0.97h 2
Carl Johannink Netherlands 3.70h 4
Javor Kac Slovenia 6.88h 19
Jakub Koukal Czech Republic 7.00h 24
Jens Lacorne France 2.14h 0
Peter Van Leuteren Netherlands 20.43h 18
Jer Nan Lou Taiwan 2.00h 1
Jer Nan Lou Taiwan 1.00h 1
Adam Marsh Australia 2.00h 4
Grigoris Maravelias Greece 0.65h 1
Pierre Martin Canada 5.90h 12
Bruce Mccurdy Canada 3.00h 6
Mukul Mhaskey India 1.50h 3
Koen Miskotte Netherlands 13.97h 11
Jurgen Rendtel Germany 18.67h 40
Alex Scholten Netherlands 2.17h 2
Rene Scurbecq Belgium 3.67h 10
Nikhil Shewale India 3.00h 3
Rohan Shewale India 3.00h 13
Wesley Stone United States 1.96h 4
Arnold Tukkers Netherlands 1.57h 2
Shigeo Uchiyama Japan 2.82h 3
Michel Vandeputte Belgium 35.38h 37
Valentin Velkov Bulgaria 8.55h 22
Amogh Waghmare India 3.00h 16
William Watson United States 3.96h 2
William Watson United States 4.91h 1
Thomas Weiland Austria 30.48h 57
Lukasz Wozniak Poland 4.00h 0
Weizhou Zeng China 1.32h 2
Desislava Zhivkova Bulgaria 3.15h 3

Data access

Create your own analysis!
Rate intervals:
nta2008_rate.csv (CSV-format).
Magnitude distributions: nta2008_magn.csv (CSV-format).