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Re: (meteorobs) AUR Obs. on Aug 31, 1999.
Thanks for sharing your observations with us. The Alpha Aurigids are
very sparse in numbers away from the night of maximum activity. With the
low limiting magnitude seeing one member during 75 minutes of observing
sounds normal to me.
Bob Lunsford
"Hashimoto, Takema" wrote:
>
> Hi All,
>
> I have just finished the observation of AUR.
> But I don't see the especially activity during obsevation.
>
> Clear skies. Takema,
>
> ===============================================================================
> AUR Observation in 1999
>
> Observation Period:
> August 31 - September 1, 1999.
>
> Observation site:
> A : Hachioji ,Tokyo, Japan 139d22m , +35d38m
>
> Observers (E-mail) :
> Takema Hashimoto : HASTA (thashi@din.or.jp)
>
> Conditions:
> Very clear sky under the moon light. But I covered a moon with my hand.
>
> Observation method:
> Visual , Plotting
>
> Observational Data:
> Date UT Time Total Spor. AUR Lm Cl Dir Obs. Site
> ----------------------------------------------------------
> Aug/1999
> 31/01 17:15-18:30 75 9 8 1 4.8 0 Per HASTA A
>
> Time : Observed time interval
> Total: Total number of meteors
> Spor.: Number of Sporadic meteors
> Lm : Limiting magnitude of field stars
> CL : Cloud cover
> Dir : Observation direction(Z:Zenith)
>
> -----------------------------------
> thashi@din.or.jp Hashimoto, Takema
> Minor Meteor Shower Circular(MMSC)
> URL : http://www.din.or.jp/~thashi/index_E.htm
> -----------------------------------
> Nippon Meteor Society (NMS)
> Association of Meteor Observers in and around Tokyo Area (AMOTA)
> -----------------------------------
>
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