The ChipWitch

Vance Oyama, Searching for Life in Our Solar System

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Wednesday, 10 May 2023

Vance I. Oyama holds a readout from the gas chromatograph in the life detection laboratory at NASA’s Ames Research Center in this picture from April 22, 1965.

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Planetary Positions

28.12.2024 at 01:26:08 UTC

chart wheel

Planet	Longitude
The Sun	06 Cap 47' 47"
The Moon	02 Sag 55' 06"
Mercury	15 Sag 02' 16"
Venus	23 Aqu 26' 45"
Mars	03 Leo 07' 39" R
Jupiter	13 Gem 39' 08" R
Saturn	14 Pis 14' 12"
Uranus	23 Tau 44' 14" R
Neptune	27 Pis 14' 52"
Pluto	00 Aqu 56' 43"

Solar Status

BZ Status:	0
Proton Density:	2.82
Proton Speed:	283.3 k/sec
KP Status:	0.67

Type	Dec 28	Dec 29	Dec 30
Active	25%	25%	25%
Minor	5%	5%	5%
Moderate	1%	1%	1%
Strong	1%	1%	1%
Kp Index Prediction
00-03UT	2.67	2.33	2.67
03-06UT	3.00	2.00	2.67
06-09UT	2.00	2.33	2.00
09-12UT	1.33	2.33	1.33
12-15UT	1.67	2.33	1.67
15-18UT	1.67	2.33	2.33
18-21UT	2.00	3.00	2.00
21-00UT	2.33	2.67	2.33
Solar Activity
Solar activity reached moderate levels. Region 3928 (S12W50, Dai/beta-gamma) produced a M1.2 flare at 27/1538 UTC as it underwent decay in its trailing spots. Region 3932 (S17W23, Dac/beta-gamma-delta) was the culprit of a C9.5 flare event at 27/0805 UTC and gained additional spots. Region 3933 (S07W48, Dac/beta-gamma) consolidated its leading spots and Region 3936 (N14W16, Ekc/beta-delta) underwent evolution as it grew in length, gaining additional spots in its intermediate area. Region 3938 (N19E25, Dac/beta-gamma) produced an M3.3 flare at 27/2035 UTC, which was the largest of the period. Regions 3940 (S05E38, Axx/alpha) and 3941 (S05E50, Hax/alpha) were numbered this period, but were otherwise unremarkable.
Solar Wind
Solar wind parameters were at nominal levels. Total field ranged 3-5 nT and the Bz component was +/- 4 nT. Solar wind speeds gradually decreased over the course of the period to near 300 km/s. Phi was predominantly negative while undertaking brief excursions into a positive orientation.
Energetic Particle
The greater than 10 MeV proton flux remained elevated above background but well below the S1 threshold. The greater than 2 MeV electron flux reached moderate levels.

Solar Monitor

Solar Wind

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