Evolution of ionospheric multicell convection during northward interplanetary magnetic field with |<i>B<sub>z</sub></i>/<i>B<sub>y</sub></i>| > 1
Bibliographic record
Abstract
During northward interplanetary magnetic field (IMF), it is generally believed that ionospheric convection appears as a four‐cell structure for | B z / B y | > 1 and as a distorted two‐cell structure for | B z / B y | < 1, where B y and B z are the Y and Z components of the IMF. In this paper we present Super Dual Auroral Radar Network (SuperDARN) observations of ionospheric convection in the Northern Hemisphere during northward IMF for | B z / B y | > 1 on November 11, 1998. We show in detail the evolution of the convection patterns as | B z / B y | changes. Nearly symmetric four‐cell convection, with two reverse cells in the polar cap and two normal cells at lower latitudes, occurs for | B z / B y | ≈ 7. The ionospheric flow associated with the reverse cells is closed almost completely on the dayside. A shifted four‐cell convection pattern, with the reverse cells shifted toward earlier magnetic local time (MLT) for negative B y and toward later MLT for positive B y , is observed for | B z / B y | ≈ 2.3. When | B z / B y | decreases to ∼1.7, the convection appears as a three‐cell pattern, with a single reverse cell focused near noon and two normal cells. The normal morning and afternoon cells are focused at quite high magnetic latitudes (between 76° and 80°); the spatial extent of the normal cells is 10°–15° or 1000–1500 km in the latitudinal direction. We also present Defense Meteorological Satellite Program (DMSP) satellite data which show sunward convection over the polar cap in the Southern Hemisphere at the same time as the Northern Hemisphere radar observations. We propose a new model of convection patterns during northward IMF for | B z / B y | > 1 and B y < 0 on the basis of the combined observations. In the model the convection appears as a symmetric four‐cell structure for | B z / B y | ≥ 3, a shifted four‐cell structure for | B z / B y | = 2–3, and a three‐cell structure for | B z / B y | = 1–2.
Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.
How this classification was reachedexpand
Full frame distilled prediction
Teacher imitationNot calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.
Codex and Gemma teacher scores by category
| Category | Codex | Gemma |
|---|---|---|
| Metaresearch | 0.000 | 0.000 |
| Meta-epidemiology (narrow) | 0.000 | 0.000 |
| Meta-epidemiology (broad) | 0.001 | 0.000 |
| Bibliometrics | 0.000 | 0.001 |
| Science and technology studies | 0.000 | 0.000 |
| Scholarly communication | 0.000 | 0.001 |
| Open science | 0.001 | 0.000 |
| Research integrity | 0.000 | 0.001 |
| Insufficient payload (model declined to judge) | 0.001 | 0.000 |
Machine scores (provisional)
The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.
Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.
score_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from itClassification
machine, unvalidatedMachine predicted; a candidate call from one teacher head, not a consensus.
How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".