Ageira Innovations - Flight Logs

[Clarissa Fairchild]

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Flight Log: Clarissa Fairchild, Ageira~Oort

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This is the second report from Munich survey mission. This time it was long range observation flight to the outer edge of heliopause of Munich sun. The goal is to explore configuration of dark matter clouds in the system.

The cloud of dark matter that engulfs Munich assumed form of sphere, approx. 80K radius with a center on the Munich main star. The cloud contains no larger bodies, but emits intense radiation. The spectral analysis of the radiation is usual for the dark matter nebulae.

The cloud itself doesn't seem homogeneous upon initial analysis. There are turbulent zones with varied density of dark matter particles and intensity of radiation. The form of the cloud and the streams observed within it make it evident that the dark matter masses were dragged by the gravity of the central star and formed a kind of maelstrom, with the dark matter moving around the start in spiral.

During two dives into the cloud, we measured the radiation, density gradients and relative speeds of different parts of the maelstrom.



824-06-24 06:01 45K to zenith from Neu Augsburg Outpost. Inside the dark matter cloud. Radiation A = 12*10^8 Bq
824-06-24 06:05 135K to zenith from Neu Augsburg. Outside the main cloud formation.
824-06-24 06:06 Walker nebula observed through secondary outcroppings of the cloud for spectral analysis.
824-06-24 06:07 Moving on to waypoint #1 in Schwarzwald cloud.
824-06-24 06:10 95K to waypoint. Close to the upper boundary of the dark matter cloud. Edge nebula observed through cloud matter for spectral analysis.
824-06-24 06:11 External radius of the cloud ~80K from the main star of Munich system.
824-06-24 06:12 Particles of dark matter on spectral scanners in external layers of the upper region of the cloud.
824-06-24 06:15 Internal radius of the dark matter cloud ~45K from the main star. Particles of dark matter observed by spectral scanners.
824-06-24 06:19 On the waypoint #1. A = 7.3*10^8 Bq.
824-06-24 06:25 External radius of the nadir portion of the cloud is ~80K from the central star.
824-06-24 06:28 Both stars of Munich system observed through the dark matter cloud for spectral analysis of the dark matter.
824-06-24 06:33 Internal border of the cloud at ~30K from the main star. A = 9.1*10^8 Bq.


Clarissa Fairchild,
Ageira Innovations