Clustering Wind data at 1 AU to contextualize magnetic reconnection in the solar wind

Open Access

Table 3.

Xu & Borovsky (2015) classification criteria.

Category	Condition
Ejecta	${log}_{10} V_{A} > 0.277 {log}_{10} S_{p} + 0.055 {log}_{10} (\frac{T_{\exp}}{T_{p}}) + 1.83$ $\log_{10} V_A > 0.277 \log_{10} S_p + 0.055 \log_{10} \left( \frac{T_{exp}}{T_p} \right) + 1.83$

Coronal Hole (CH)	${log}_{10} (S_{p}) > - 0.525 {log}_{10} (\frac{T_{\exp}}{T_{p}}) - 0.676 {log}_{10} (V_{A}) + 1.74$ $\log_{10}(S_p) > -0.525 \log_{10} \left( \frac{T_{exp}}{T_p} \right) - 0.676 \log_{10}(V_A) + 1.74$ and not classified as Ejecta

Sector Reversal (SR)	${log}_{10} (S_{p}) < - 0.658 {log}_{10} (V_{A}) - 0.125 {log}_{10} (\frac{T_{\exp}}{T_{p}}) + 1.04$ $\log_{10}(S_p) < -0.658 \log_{10}(V_A) - 0.125 \log_{10} \left( \frac{T_{exp}}{T_p} \right) + 1.04$ and not classified as Ejecta

Streamer Belt (SB)	Remaining data points not satisfying any of the above conditions

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.