Credit: Me :D
Credit: Me :D

Where do meteoroids come from?
Rosetta OSIRIS - 67P/Churyumov-Gerasimenko
Shigaraki Middle and Upper Atmosphere (MU) radar, Japan
Reliably investigate
Apply on multiple radar systems
pipeline
model parameter estimation
Bayes' theorem
$$ P(\text{model} | \text{data}) = \frac{P(\text{data} | \text{model}) P(\text{model})}{P(\text{data})} $$
pipeline
(Kastinen, D., Kero, J., 2022a.)
Some other upgrades:
new analysis
new analysis
Kastinen, D., Kero, J., 2022a.
new analysis
Credit: Wikimedia Commons (Seahen)
new analysis
Credit: Wikimedia Commons (Lasunncty)
high-altitude detections
high-altitude detections
516 out of 106,000 events
high-altitude detections
(Kastinen, D., Kero, J., 2022b.)
high-altitude detections
(Kastinen, D., Kero, J., 2022b.)
high-altitude detections
(Kastinen, D., Kero, J., 2022b.)
high-altitude detections
group-D (soft cometary material): $k_b$ < 6.6
high-altitude detections
"manual correction"
January zeta-Leonids
What is space debris?
ESA - Time to act
ESA - Time to act
KOSMOS-1408
C. Space debris
Kosmos-1408 destruction:
Russian anti-satellite weapon
Credit: AstroDyn on YouTube
C. Space debris
VIII.
Kastinen, D.,Vierinen J.,Grydeland T.,Kero J., 2022.
C. Space debris
VIII.
Kastinen, D.,Vierinen J.,Grydeland T.,Kero J., 2022.
New size estimation method
| metecho | Meteor head echo analysis | [transferring] |
| htpl | Radar hard target processing lib | [refactoring] |
| pyorb | Kepler to cartesian elements | on PyPI |
| pyant | Radar antenna radiation patterns | on PyPI |
| ablate | Ablation model interfaces | [ongoing] |
| pyod | Orbit determination interfaces | [ongoing] |
| dasst | Meteoroid stream simulations | [Only prototype] |
Photo: EISCAT
Photo: EISCAT
Photo: EISCAT
Technical information