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Merge pull request #37 from davesrocketshop/dev2.8
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Fin flutter
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davesrocketshop authored Sep 18, 2022
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131 changes: 131 additions & 0 deletions Analyzers/FinFlutter.py
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# ***************************************************************************
# * Copyright (c) 2022 David Carter <[email protected]> *
# * *
# * This program is free software; you can redistribute it and/or modify *
# * it under the terms of the GNU Lesser General Public License (LGPL) *
# * as published by the Free Software Foundation; either version 2 of *
# * the License, or (at your option) any later version. *
# * for detail see the LICENCE text file. *
# * *
# * This program is distributed in the hope that it will be useful, *
# * but WITHOUT ANY WARRANTY; without even the implied warranty of *
# * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the *
# * GNU Library General Public License for more details. *
# * *
# * You should have received a copy of the GNU Library General Public *
# * License along with this program; if not, write to the Free Software *
# * Foundation, Inc., 59 Temple Place, Suite 330, Boston, MA 02111-1307 *
# * USA *
# * *
# ***************************************************************************
"""Class for analyzing fin flutter"""

__title__ = "FreeCAD Fin Flutter Analyzer"
__author__ = "David Carter"
__url__ = "https://www.davesrocketshop.com"

import math

from DraftTools import translate

from Analyzers.pyatmos import coesa76
from Analyzers.pyatmos.utils.Const import p0, gamma, R_air

from App.Constants import FIN_TYPE_TRAPEZOID, FIN_TYPE_ELLIPSE

class FinFlutter:

def __init__(self, fin):
self._fin = fin

if fin.FinType == FIN_TYPE_TRAPEZOID:

# Convert from mm to m
self._tipChord = float(fin.TipChord) / 1000.0
self._rootChord = float(fin.RootChord) / 1000.0
self._thickness = float(fin.RootThickness) / 1000.0
self._span = float(fin.Height) / 1000.0

self._area = (self._rootChord + self._tipChord) * self._span / 2.0
elif fin.FinType == FIN_TYPE_ELLIPSE:
raise TypeError(translate('Rocket', "Elliptical fins are not supported at this time"))

# # Convert from mm to m
# self._tipChord = 0.0
# self._rootChord = float(fin.RootChord) / 1000.0
# self._thickness = float(fin.RootThickness) / 1000.0
# self._span = float(fin.Height) / 1000.0

# self._area = math.pi * (self._rootChord / 2.0) * self._span
else:
raise TypeError(translate('Rocket', "Custom fins are not supported at this time"))

self._aspectRatio = self._span**2 / self._area
self._lambda = self._tipChord / self._rootChord


def shearModulus(self, young, poisson):
return young / (2.0 * (1.0 + poisson))

def atmosphericConditions(self, altitude):

# Get the atmospheric conditions at the specified altitude (convert mm to km)
# Uses the coesa76 model which is an extension of US Standard Atmosphere 1976 model to work above 84K
atmo = coesa76([altitude / (1000.0 * 1000.0)])

temp = atmo.T
pressure = atmo.P

# speed of sound
a = math.sqrt(gamma * R_air * temp)

return a,pressure

def flutter(self, altitude, shear):
# Calculate fin flutter using the method outlined in NACA Technical Note 4197

a,pressure = self.atmosphericConditions(altitude)

shear *= 1000.0 # Convert from kPa to Pa

# The coefficient is adjusted for SI units
Vf = math.sqrt(shear / ((270964.068 * (self._aspectRatio**3)) / (pow(self._thickness / self._rootChord, 3) * (self._aspectRatio + 2)) * ((self._lambda + 1) / 2) * (pressure / p0)))

# Flutter velocity in m/s
Vfa = a * Vf

return Vf, Vfa

def flutterPOF(self, altitude, shear):
#
# Calculate flutter using the formula outlined in Peak of Flight issue 291
# There is some discussion that this may over estimate the flutter by a factor of sqrt(2) vs the NACA method
#

a,pressure = self.atmosphericConditions(altitude)

shear *= 1000.0 # Convert from kPa to Pa

# Flutter velocity in Mach
Vf = math.sqrt((shear * 2 * (self._aspectRatio + 2) * pow(self._thickness / self._rootChord, 3)) / (1.337 * pow(self._aspectRatio, 3) * pressure * (self._lambda + 1)))

# Flutter velocity in m/s
Vfa = a * Vf

return Vf, Vfa

def divergence(self, altitude, shear):
# Calculate fin divergence using the method outlined in NACA Technical Note 4197

a,pressure = self.atmosphericConditions(altitude)

shear *= 1000.0 # Convert from kPa to Pa

# Divergent velocity in Mach
Vd = math.sqrt(shear / (((3.3 * pressure) / (1 + (2 / self._aspectRatio))) * ((self._rootChord + self._tipChord) / self._thickness**3) * (self._span**2)))

# Divergent velocity in m/s
Vda = a * Vd

return Vd, Vda

21 changes: 21 additions & 0 deletions Analyzers/pyatmos/LICENSE.txt
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MIT License

Copyright (c) 2019-2021 Chunxiao Li

Permission is hereby granted, free of charge, to any person obtaining a copy
of this software and associated documentation files (the "Software"), to deal
in the Software without restriction, including without limitation the rights
to use, copy, modify, merge, publish, distribute, sublicense, and/or sell
copies of the Software, and to permit persons to whom the Software is
furnished to do so, subject to the following conditions:

The above copyright notice and this permission notice shall be included in all
copies or substantial portions of the Software.

THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND, EXPRESS OR
IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF MERCHANTABILITY,
FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT. IN NO EVENT SHALL THE
AUTHORS OR COPYRIGHT HOLDERS BE LIABLE FOR ANY CLAIM, DAMAGES OR OTHER
LIABILITY, WHETHER IN AN ACTION OF CONTRACT, TORT OR OTHERWISE, ARISING FROM,
OUT OF OR IN CONNECTION WITH THE SOFTWARE OR THE USE OR OTHER DEALINGS IN THE
SOFTWARE.
161 changes: 161 additions & 0 deletions Analyzers/pyatmos/README.md
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# Welcome to ATMOS

[![PyPI version shields.io](https://img.shields.io/pypi/v/pyatmos.svg)](https://pypi.python.org/pypi/pyatmos/) [![PyPI pyversions](https://img.shields.io/pypi/pyversions/pyatmos.svg)](https://pypi.python.org/pypi/pyatmos/) [![PyPI status](https://img.shields.io/pypi/status/pyatmos.svg)](https://pypi.python.org/pypi/pyatmos/) [![GitHub contributors](https://img.shields.io/github/contributors/lcx366/ATMOS.svg)](https://GitHub.com/lcx366/ATMOS/graphs/contributors/) [![Maintenance](https://img.shields.io/badge/Maintained%3F-yes-green.svg)](https://GitHub.com/lcx366/ATMOS/graphs/commit-activity) [![GitHub license](https://img.shields.io/github/license/lcx366/ATMOS.svg)](https://github.com/lcx366/ATMOS/blob/master/LICENSE) [![Documentation Status](https://readthedocs.org/projects/pystmos/badge/?version=latest)](http://pyatmos.readthedocs.io/?badge=latest)

This package is an archive of scientific routines that estimates the vertical structure of atmosphere with various *atmospheric density models*, such as **Exponential**(-0.611\~1000 km), **COESA76**(-0.611\~1000 km), **NRLMSISE-00**(0\~2000 km), and **JB2008**(90\~2500 km).

The **NRLMSISE-00** model was developed by the US Naval Research Laboratory. It is based on mass spectrometry and incoherent radar scatter data, also incorporates drag and accelerometer data, and accounts for anomalous oxygen at high altitudes(>500 km). It is recommended by the International Committee on Space Resarch (COSPAR) as the standard for atmospheric composition. Two indices are used in this model: *F10.7* (both the daily solar flux value of the previous day and the 81-day average centred on the input day) and $A_p$ (geomagnetic daily value).

The **JB2008** (Jacchia-Bowman) model is a newer model developed by Space Environment Technologies(SET) and the US Air Force Space Command. The model accounts for various phenomena related to EUV heating of the thermosphere and uses the DST index as the driver of global density changes. The model is complementary to the NRLMSISE00 model and is more accurate during times of high solar activity and geomagnetic storms. It is recommended by COSPAR as the standard for thermospheric density in satellite drag calculations. Four solar indices and two geomagnetic activity indices are used in this model: *F10.7* (both tabular value one day earlier and the 81-day average centred on the input time); *S10.7* (both tabular value one day earlier and the 81-day average centred on the input time); *M10.7* (both tabular value five days earlier and the 81-day average centred on the input time); Y10.7 (both tabular value five days earlier and the 81-day average centred on the input time); $a_p$ (3 hour tabular value); and *DST* (converted and input as a dTc temperature change tabular value on the input time).

The **Exponential** returns

- the mass density

The **COESA76** returns

- the mass density, temperature, and pressure at the altitude

The **NRLMSISE-00** returns

- the number densities of atmospheric constituents including N$_2$, O$_2$, Ar, He, O, N, and anomalous oxygen at altitude above 500 km

- the temperature at the altitude

- the total mass density including the anomalous oxygen component

The **JB2008** returns

- the temperature at the altitude

- the total mass density

## How to install

On Linux, macOS and Windows architectures, the binary wheels can be installed using **pip** by executing one of the following commands:

```sh
pip install pyatmos
pip install pyatmos --upgrade # to upgrade a pre-existing installation
```

## How to use

#### Exponential

```python
>>> from pyatmos import expo
>>> expo_geom = expo([0,20,40,60,80]) # geometric altitudes by default
>>> print(expo_geom.rho) # [kg/m^3]
>>> # expo_geop = expo([0,20,40,60,80],'geopotential') # geopotential altitudes

[1.22500000e+00 7.76098911e-02 3.97200000e-03 3.20600000e-04
1.90500000e-05]
```

#### COESA 1976

```python
>>> from pyatmos import coesa76
>>> coesa76_geom = coesa76([0,20,40,60,80]) # geometric altitudes by default
>>> print(coesa76_geom.rho) # [kg/m^3]
>>> print(coesa76_geom.T) # [K]
>>> print(coesa76_geom.P) # [Pa]
>>> # coesa76_geop = coesa76([0,20,40,60,80],'geopotential') # geopotential altitudes

[1.22499916e+00 8.89079563e-02 3.99535051e-03 3.09628985e-04
1.84514759e-05]
[288.15 216.65 250.35120115 247.01740767 198.63418825]
[1.01325000e+05 5.52919008e+03 2.87122194e+02 2.19548951e+01
1.05207648e+00]
```

#### NRLMSISE-00

*Before using NRLMSISE-00, the space weather data needs to be prepared in advance.*

```python
>>> from pyatmos import download_sw_nrlmsise00,read_sw_nrlmsise00
>>> # Download or update the space weather file from www.celestrak.com
>>> swfile = download_sw_nrlmsise00()
>>> # Read the space weather data
>>> swdata = read_sw_nrlmsise00(swfile)
```

```python
>>> from pyatmos import nrlmsise00
>>> # Set a specific time and location
>>> t = '2014-07-22 22:18:45' # time(UTC)
>>> lat,lon,alt = 25,102,600 # latitude, longitude in [degree], and altitude in [km]
>>> nrl00 = nrlmsise00(t,(lat,lon,alt),swdata)
>>> print(nrl00.rho) # [kg/m^3]
>>> print(nrl00.T) # [K]
>>> print(nrl00.nd) # composition in [1/m^3]

1.714115212984513e-14
765.8976564552341
{'He': 645851224907.2849, 'O': 456706971423.5056, 'N2': 531545420.00015724, 'O2': 2681352.1654067687, 'Ar': 406.9308900607773, 'H': 157249711103.90558, 'N': 6759664327.87355, 'ANM O': 10526544596.059282}
```

#### JB2008

*Before using JB2008, the space weather data needs to be prepared in advance.*

```python
>>> from pyatmos import download_sw_jb2008,read_sw_jb2008
>>> # Download or update the space weather file from https://sol.spacenvironment.net
>>> swfile = download_sw_jb2008()
>>> # Read the space weather data
>>> swdata = read_sw_jb2008(swfile)
```

```python
>>> from pyatmos import jb2008
>>> # Set a specific time and location
>>> t = '2014-07-22 22:18:45' # time(UTC)
>>> lat,lon,alt = 25,102,600 # latitude, longitude in [degree], and altitude in [km]
>>> jb08 = jb2008(t,(lat,lon,alt),swdata)
>>> print(jb08.rho) # [kg/m^3]
>>> print(jb08.T) # [K]

1.2991711750265394e-14
754.2803276187265
```

## Change log
- **1.2.3 — Jun 7, 2021**
- Added atmospheric models **JB2008**
- Changed the output of the result to an instance
- Improved the code structure for NRLMSISE-00, and the running speed is nearly threefold
- **1.2.1 — Jan 22, 2021**
- Added **Exponential Atmosphere** up to 1000 km
- Added **Committee on Extension to the Standard Atmosphere(COESA)** up to 1000 km
- Completed part of the help documentation for NRLMSISE-00
- Improved the code structure to make it easier to read
- **1.1.2 — Jul 26, 2020**
- Added colored-progress bar for downloading data
- **1.1.0 — Mar 29, 2020**
- Added the International Standard Atmosphere(ISA) Model up to 86kms

## Next release

- Because there is a **45-day lag** between the current Day-Of-Year and the last data DOY in the indices files provided by Space Environment Technologies(SET), the forecasts through the last data DOY out to 137 days (5 solar rotations) need to be estimated using machine learning or other methods.
- Add other atmospheric models, such as the **Earth Global Reference Atmospheric Model(Earth-GRAM) 2016**, and the **Drag Temperature Model(DTM)2013**.

## Reference

- U.S. Standard Atmosphere, 1976, U.S. Government Printing Office, Washington, D.C.
- [Public Domain Aeronautical Software](http://www.pdas.com/atmos.html)
- https://gist.github.com/buzzerrookie/5b6438c603eabf13d07e
- https://ww2.mathworks.cn/help/aerotbx/ug/atmosisa.html
- [Original Fortran and C code](https://ccmc.gsfc.nasa.gov/pub/modelweb/atmospheric/msis/)
- [MSISE-00 in Python and Matlab](https://github.com/space-physics/msise00)
- [NRLMSISE-00 Atmosphere Model - Matlab](https://ww2.mathworks.cn/matlabcentral/fileexchange/56253-nrlmsise-00-atmosphere-model?requestedDomain=zh)
- [NRLMSISE-00 Atmosphere Model - Aerospace Blockset](https://www.mathworks.com/help/aeroblks/nrlmsise00atmospheremodel.html?requestedDomain=)
- [NRLMSISE-00 Atmosphere Model - CCMC](https://ccmc.gsfc.nasa.gov/modelweb/models/nrlmsise00.php)
- [NRLMSISE-00 empirical model of the atmosphere: Statistical comparisons and scientific issues](http://onlinelibrary.wiley.com/doi/10.1029/2002JA009430/pdf)
- [ATMOSPHERIC MODELS](http://www.braeunig.us/space/atmmodel.htm)
- [poliastro-Atmosphere module](https://docs.poliastro.space/en/latest/autoapi/poliastro/earth/atmosphere/index.html?highlight=poliastro.earth.atmosphere)
- [ATMOSPHERE API](https://amentum.com.au/atmosphere)
- [COSPAR International Reference Atmosphere - 2012](https://spacewx.com/wp-content/uploads/2021/03/chapters_1_3.pdf)

10 changes: 10 additions & 0 deletions Analyzers/pyatmos/__init__.py
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'''
pyatmos package
This package is an archive of scientific routines that implement the
estimation of atmospheric properties for various atmospheric models, such
as exponential, coesa76, nrlmsise00, and jb2008.
'''

from .standardatmos.coesa76 import coesa76
17 changes: 17 additions & 0 deletions Analyzers/pyatmos/class_atmos.py
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class ATMOS(object):
'''
class ATMOS
- attributes:
- self defined
- methods:
- None
'''
def __init__(self,info):
self.info = info

for key in info.keys():
setattr(self, key, info[key])

def __repr__(self):
return 'Instance of class ATMOS'
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6 changes: 6 additions & 0 deletions Analyzers/pyatmos/data/readme.txt
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coesa76_coeffs.npz:

Coefficients of equations from which the pressure and density for geometric altitudes from 86 km to 1000 km are computed. The basic equation form is EXP( A × z^4 + B × z^3 + C × z^2 + D × z + E )
More info to see http://www.braeunig.us/space/atmmodel.htm#USSA1976

nrlmsis00_data.npz:
15 changes: 15 additions & 0 deletions Analyzers/pyatmos/standardatmos/__init__.py
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'''
Standard Atmosphere Model
This subpackage defines the following functions:
expo.py
expo - Estimate the air densities at given geometric or geopotential altitudes
above the sea level using a exponential atmosphere model.
ussa76.py
lapse_tp - Calculate the temperature and pressure at a given geopotential altitude above base of a specific layer.
ussa76 - Implements the U.S. Standard Atmosphere 1976(USSA76) up to 86km.
coesa76.py
coesa76 - Implements the U.S. Committee on Extension to the Standard Atmosphere(COESA 1976) up to 1000km.
'''
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