Artemis II Crew’s SLS Visit

Images

Thursday, 07 December 2023

Artemis II NASA astronauts Reid Wiseman (left) and Christina Koch (middle) of NASA and CSA (Canadian Space Agency) astronaut Jeremy Hansen (second from left) view the core stage for the Space Launch System rocket at the agency’s Michoud Assembly Facility in New Orleans on Nov. 16. The three astronauts, along with NASA’s Victor Glover, will launch atop the rocket stage to venture around the Moon on Artemis II, the first crewed flight for Artemis.

Image Credit: NASA / Michael DeMocker

Planetary Positions

27.04.2024 at 12:37:06 UTC

Planet	Longitude
The Sun	07 Tau 44' 17"
The Moon	18 Sag 36' 06"
Mercury	16 Ari 08' 38"
Venus	27 Ari 35' 30"
Mars	27 Pis 35' 29"
Jupiter	23 Tau 18' 48"
Saturn	16 Pis 19' 39"
Uranus	22 Tau 11' 23"
Neptune	28 Pis 49' 23"
Pluto	02 Aqu 05' 50"

Solar Status

BZ Status:	-8
Proton Density:	1.84
Proton Speed:	442.9 k/sec
KP Status:	1.33

Type	Apr 27	Apr 28	Apr 29
Active	35%	35%	25%
Minor	25%	20%	10%
Moderate	10%	5%	1%
Strong	1%	1%	1%
Kp Index Prediction
00-03UT	3.67	3.67	2.67
03-06UT	3.00	3.33	2.00
06-09UT	3.00	3.33	2.33
09-12UT	3.00	3.00	2.67
12-15UT	3.00	3.00	2.33
15-18UT	3.33	3.33	2.33
18-21UT	3.33	2.00	2.33
21-00UT	3.67	2.00	2.33
Solar Activity
Solar activity declined to low levels this period with only C-class flare activity observed. Region 3654 (S08W16, Ehi/beta-gamma) remained the largest region on the disk and exhibited moderate development in the intermediate and trailer spots. Region 3657 (S15W25, Bxo/beta) reemerged with a few rudimentary spots and new Region 3660 (N10E71, Axx/alpha) was numbered. The remaining regions were either stable or in decay. No Earth-directed CMEs were detected in available imagery.
Solar Wind
The solar wind environment was enhanced due to likely CME activity early in the period, followed by the onset of positive polarity CH HSS influences. Total field strength reached a peak of 17 nT and the Bz component was sustained southward through the first half of the period, with a peak deflection of -11 nT observed. During the latter half of the period, the Bz component rotated northward with only brief southward deflections observed. Solar wind speeds were steady between 300-350 km/s until 27/0230 UTC, when speed values slowly increased to a period high of around 550 km/s. The phi angle transitioned from negative to positive at 26/1502 UTC.
Energetic Particle
The greater than 2 MeV electron flux was at normal to moderate levels and the greater than 10 MeV proton flux was steady at background levels.

Artemis II Crew’s SLS Visit

Related Posts

Hubble Spots a Magnificent Barred Galaxy

Navigating the Moon with Art

Tracking Spring Flooding

Hubble Spots the Little Dumbbell Nebula

Our Beautiful Water World