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Velocity-modified Cylindrical Flux Rope Model for Magnetic Clouds (MC)




1. Your information (which is used to notify you when the submitted job is done):
	Name:
	Email:

2. Choose model:
		Gold & Hoyle [1960] solution: A non-linear force-free flux rope with uniform-twist magnetic field lines
			[Wang et al., JGR, 121, 9316-9339, 2016]
		Lundquist [1950] solution: A linear force-free flux rope
			[Wang et al., JGR, 120, 1543-1565, 2015]

3. Select data source:
	Use the local data (Please specify the spacecraft, the data and time below).
		Spacecraft:		Wind, ACE
		The Begin and End time of the interval of interest must cover the interval of the MC to be fitted.
		Begin:		(YYYY/MM/DD HH:MM:SS)
		End:		(YYYY/MM/DD HH:MM:SS)
	Use your own data (see *description* of the data format). You will be able to upload your own data at the next step.

4. Set the boundary of the MC to be fitted:

	Begin:			(YYYY/MM/DD HH:MM:SS)
	End:			(YYYY/MM/DD HH:MM:SS)

5.^* Set fitting options:
	Time resolution:			s (at least 300 s)
	Degree step:			deg (at least 15 deg)
	Velocity:			on, off



Note: * means optional. To report a bug, send an email to Dr. Yuming Wang.

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