-
Notifications
You must be signed in to change notification settings - Fork 3
Home
Welcome to the Perception-Project wiki! Udacity - Robotics NanoDegree Program
Project code file is consisting of the following major parts:
- Required python imports
- helper functions
- pcl_callback() function
- pr2_mover function
- Creating ROS Node, Subscribers, and Publishers
I will be explaning each part in this writeup.
In this project we used multiple python libraries including:
- numpy: for mathematics
- sklearn: for SVM machine learning
- pickle: to dump/load data to disk files
- yaml: to generate yaml format and write it to disk.
Some of the ROS libraries:
- rospy: ROS python library
- tf: ROS transforms library
- ros visualization_msgs: ROS marker visualization library
- ros messages formats and converters.
and functions from sensor_stick exercises.
import numpy as np
import sklearn
from sklearn.preprocessing import LabelEncoder
import pickle
from sensor_stick.srv import GetNormals
from sensor_stick.features import compute_color_histograms
from sensor_stick.features import compute_normal_histograms
from visualization_msgs.msg import Marker
from sensor_stick.marker_tools import *
from sensor_stick.msg import DetectedObjectsArray
from sensor_stick.msg import DetectedObject
from sensor_stick.pcl_helper import *
import rospy
import tf
from geometry_msgs.msg import Pose
from std_msgs.msg import Float64
from std_msgs.msg import Int32
from std_msgs.msg import String
from pr2_robot.srv import *
from rospy_message_converter import message_converter
import yaml
# Helper function to get surface normals
def get_normals(cloud):
get_normals_prox = rospy.ServiceProxy('/feature_extractor/get_normals', GetNormals)
return get_normals_prox(cloud).cluster
# Helper function to create a yaml friendly dictionary from ROS messages
def make_yaml_dict(test_scene_num, arm_name, object_name, pick_pose, place_pose):
yaml_dict = {}
yaml_dict["test_scene_num"] = test_scene_num.data
yaml_dict["arm_name"] = arm_name.data
yaml_dict["object_name"] = object_name.data
yaml_dict["pick_pose"] = message_converter.convert_ros_message_to_dictionary(pick_pose)
yaml_dict["place_pose"] = message_converter.convert_ros_message_to_dictionary(place_pose)
return yaml_dict
# Helper function to output to yaml file
def send_to_yaml(yaml_filename, yaml_dict_list):
data_dict = {"object_list": yaml_dict_list}
with open(yaml_filename, 'w') as outfile:
yaml.dump(data_dict, outfile, default_flow_style=False)
# Function to search list of dictionaries and return a selected value in selected dictionary
def search_dictionaries(key1, value1, key2, list_of_dictionaries):
selected_dic = [element for element in list_of_dictionaries if element[key1] == value1][0]
selected_val = selected_dic.get(key2)
return selected_val
pcl_callback()
is the function that will be called back every time a message is published to /pr2/world/points
topic. this function has the 3D point cloud perception pipeline, object detection, and a call to the PR2 mover function.
Following sections will explain the different stages of the perception pipeline used to detect objects before starting the pick and place robot movement.
The first step in the perception pipeline is to subscribe to the the camera data (point cloud) topic /pr2/world/points
from which we will get a point cloud with noise as seen below:
before we can process the data we need to convert it from ROS PointCloud2 message to a PCL PointXYZRGB format using the following code:
cloud = ros_to_pcl(pcl_msg)
First filter is the PCL’s Statistical Outlier Removal filter. in this filter for each point in the point cloud, it computes the distance to all of its neighbors, and then calculates a mean distance. By assuming a Gaussian distribution, all points whose mean distances are outside of an interval defined by the global distances mean+standard deviation are considered to be outliers and removed from the point cloud.
Code is as following:
cloud = XYZRGB_to_XYZ(cloud)
outlier_filter = cloud.make_statistical_outlier_filter()
# Set the number of neighboring points to analyze for any given point
outlier_filter.set_mean_k(5)
# Set threshold scale factor
x = 0.0005
# Any point with a mean distance larger than global (mean distance+x*std_dev) will be considered outlier
outlier_filter.set_std_dev_mul_thresh(x)
# Finally call the filter function for magic
outliers_removed = outlier_filter.filter()
outliers_removed = XYZ_to_XYZRGB(outliers_removed,[255,255,255])
Mean K = 5 was the best value I found to almost remove all noise pixels. any value higher than 3 was leaving some of the noise pixels behind. x was selected to be 0.0005.
following image is showing result after removal of noise:
2nd stage is Voxel Grid Downsampling filter to derive a point cloud that has fewer points but should still do a good job of representing the input point cloud as a whole. This is done to reduce required computation power without impacting the final results. Code is as following:
# Create a VoxelGrid filter object for our input point cloud
vox = outliers_removed.make_voxel_grid_filter()
LEAF_SIZE = 0.005
# Set the voxel (or leaf) size
vox.set_leaf_size(LEAF_SIZE, LEAF_SIZE, LEAF_SIZE)
# Call the filter function to obtain the resultant downsampled point cloud
cloud_filtered = vox.filter()
After trying different sizes I have selected leaf size 0.005 to avoid any impact on point cloud details.
result is as shown in below image:
3rd stage is PassThrough filter which works much like a cropping tool allowing to crop any given 3D point cloud by specifying an axis with cut-off values along that axis. The region you allow to pass through, is often referred to as region of interest.
In our case I have applied the filter two times, 1st one along Z axis to select only the table top and objects on it as shown in below code:
# Create a PassThrough filter object.
passthrough = cloud_filtered.make_passthrough_filter()
# Assign axis and range to the passthrough filter object.
filter_axis = 'z'
passthrough.set_filter_field_name(filter_axis)
axis_min = 0.6
axis_max = 1.1
passthrough.set_filter_limits(axis_min, axis_max)
# Use the filter function to obtain the resultant point cloud.
cloud_filtered = passthrough.filter()
axis_min and axis_max was picked from RViz directly by reading the edge pixels values.
2nd one is along Y axis to remove the unwanted left and right edges of the table. Code is as following:
# Create a PassThrough filter object.
passthrough = cloud_filtered.make_passthrough_filter()
# Assign axis and range to the passthrough filter object.
filter_axis = 'y'
passthrough.set_filter_field_name(filter_axis)
axis_min = -0.456
axis_max = 0.456
passthrough.set_filter_limits(axis_min, axis_max)
# Use the filter function to obtain the resultant point cloud.
cloud_filtered = passthrough.filter()
again axis_min and axis_max was selected from RViz by reading the values of the edge pixels.
Next we need to remove the table itself from the scene. To do this we will use a popular technique known as Random Sample Consensus or "RANSAC". RANSAC is an algorithm, that we can use to identify points in our dataset that belong to a particular model. In the case of the 3D scene we are working with here, the model we choose could be a plane, a cylinder, a box, or any other common shape. Since the top of the table in the scene is the single most prominent plane, after ground removal, we can effectively use RANSAC to identify points that belong to the table and discard/filter out those points.
code is as following:
# Create the segmentation object
seg = cloud_filtered.make_segmenter()
# Set the model you wish to fit
seg.set_model_type(pcl.SACMODEL_PLANE)
seg.set_method_type(pcl.SAC_RANSAC)
# Max distance for a point to be considered fitting the model
# Experiment with different values for max_distance
# for segmenting the table
max_distance = 0.006
seg.set_distance_threshold(max_distance)
# Call the segment function to obtain set of inlier indices and model coefficients
inliers, coefficients = seg.segment()
# Extract inliers(Table)
cloud_table = cloud_filtered.extract(inliers, negative=False)
# Extract outliers(Objects)
cloud_objects = cloud_filtered.extract(inliers, negative=True)
Image of the objects:
Image of the table:
Last filtering step is to use PCL's Euclidean Clustering algorithm to segment the remaining points into individual objects. code is as following:
white_cloud = XYZRGB_to_XYZ(extracted_objects)
tree = white_cloud.make_kdtree()
# Create a cluster extraction object
ec = white_cloud.make_EuclideanClusterExtraction()
# Set tolerances for distance threshold
# as well as minimum and maximum cluster size (in points)
ec.set_ClusterTolerance(0.03)
ec.set_MinClusterSize(30)
ec.set_MaxClusterSize(5000)
# Search the k-d tree for clusters
ec.set_SearchMethod(tree)
# Extract indices for each of the discovered clusters
cluster_indices = ec.Extract()
Then we use the following code to add a color for each segmented object:
# Assign a color corresponding to each segmented object in scene
cluster_color = get_color_list(len(cluster_indices))
color_cluster_point_list = []
for j, indices in enumerate(cluster_indices):
for i, indice in enumerate(indices):
color_cluster_point_list.append([white_cloud[indice][0],
white_cloud[indice][1],
white_cloud[indice][2],
rgb_to_float(cluster_color[j])])
# Create new cloud containing all clusters, each with unique color
cluster_cloud = pcl.PointCloud_PointXYZRGB()
cluster_cloud.from_list(color_cluster_point_list)
resulting objects image:
Befor we can publish the processed point clouds we need to convert the format back from PCL PointXYZRGB to ROS PointCloud2 message:
pcl_msg_object = pcl_to_ros(cloud_objects)
pcl_msg_table = pcl_to_ros(cloud_table)
pcl_msg_cluster = pcl_to_ros(cluster_cloud)
finally we publish to required topics:
pcl_objects_pub.publish(pcl_msg_object)
pcl_table_pub.publish(pcl_msg_table)
pcl_cluster_pub.publish(pcl_msg_cluster)
Having the segmented objects, now we can use the SVM algorithm to predict each object. We will be using code that was developed in previous exercises:
Following are helper functions used to capture features:
def compute_color_histograms(cloud, using_hsv=False):
# Compute histograms for the clusters
point_colors_list = []
# Step through each point in the point cloud
for point in pc2.read_points(cloud, skip_nans=True):
rgb_list = float_to_rgb(point[3])
if using_hsv:
point_colors_list.append(rgb_to_hsv(rgb_list) * 255)
else:
point_colors_list.append(rgb_list)
# Populate lists with color values
channel_1_vals = []
channel_2_vals = []
channel_3_vals = []
for color in point_colors_list:
channel_1_vals.append(color[0])
channel_2_vals.append(color[1])
channel_3_vals.append(color[2])
# Compute histograms
nbins=32
bins_range=(0, 256)
# Compute the histogram of the channels separately
channel_1_hist = np.histogram(channel_1_vals, bins=nbins, range=bins_range)
channel_2_hist = np.histogram(channel_2_vals, bins=nbins, range=bins_range)
channel_3_hist = np.histogram(channel_3_vals, bins=nbins, range=bins_range)
# Concatenate the histograms into a single feature vector
hist_features = np.concatenate((channel_1_hist[0], channel_2_hist[0], channel_1_hist[0])).astype(np.float64)
# Normalize the result
normed_features = hist_features / np.sum(hist_features)
# Generate random features for demo mode.
# Replace normed_features with your feature vector
#normed_features = np.random.random(96)
# Return the feature vector
return normed_features
def compute_normal_histograms(normal_cloud):
norm_x_vals = []
norm_y_vals = []
norm_z_vals = []
for norm_component in pc2.read_points(normal_cloud,
field_names = ('normal_x', 'normal_y', 'normal_z'),
skip_nans=True):
norm_x_vals.append(norm_component[0])
norm_y_vals.append(norm_component[1])
norm_z_vals.append(norm_component[2])
# Compute histograms of normal values (just like with color)
nbins=32
bins_range=(-1, 1)
# Compute the histogram of the channels separately
norm_x_hist = np.histogram(norm_x_vals, bins=nbins, range=bins_range)
norm_y_hist = np.histogram(norm_y_vals, bins=nbins, range=bins_range)
norm_z_hist = np.histogram(norm_z_vals, bins=nbins, range=bins_range)
# Concatenate the histograms into a single feature vector
hist_features = np.concatenate((norm_x_hist[0], norm_y_hist[0], norm_z_hist[0])).astype(np.float64)
# Normalize the result
normed_features = hist_features / np.sum(hist_features)
# Generate random features for demo mode.
# Replace normed_features with your feature vector
#normed_features = np.random.random(96)
return normed_features
Full code for capturing features and training SVM:
Code to detect the objects using above functions:
detected_objects_labels = []
detected_objects = []
for index, pts_list in enumerate(cluster_indices):
#----------------------------------------------------------------------------------
# Grab the points for the cluster from the extracted_objects
#----------------------------------------------------------------------------------
pcl_cluster = extracted_objects.extract(pts_list)
# Convert the cluster from pcl to ROS using helper function
ros_cluster = pcl_to_ros(pcl_cluster)
#----------------------------------------------------------------------------------
# Generate Histograms
#----------------------------------------------------------------------------------
# Color Histogram
c_hists = compute_color_histograms(ros_cluster, using_hsv=True)
# Normals Histogram
normals = get_normals(ros_cluster)
n_hists = compute_normal_histograms(normals)
#----------------------------------------------------------------------------------
# Generate feature by concatenate of color and normals.
#----------------------------------------------------------------------------------
feature = np.concatenate((c_hists, n_hists))
#----------------------------------------------------------------------------------
# Make the prediction
#----------------------------------------------------------------------------------
# Retrieve the label for the result and add it to detected_objects_labels list
prediction = clf.predict(scaler.transform(feature.reshape(1,-1)))
label = encoder.inverse_transform(prediction)[0]
detected_objects_labels.append(label)
#----------------------------------------------------------------------------------
# Publish a label into RViz
#----------------------------------------------------------------------------------
label_pos = list(white_cloud[pts_list[0]])
label_pos[2] += .2
object_markers_pub.publish(make_label(label,label_pos, index))
# Add the detected object to the list of detected objects.
#----------------------------------------------------------------------------------
do = DetectedObject()
do.label = label
do.cloud = ros_cluster
detected_objects.append(do)
rospy.loginfo('Detected {} objects: {}'.format(len(detected_objects_labels), detected_objects_labels))
#----------------------------------------------------------------------------------
# Publish the list of detected objects
#----------------------------------------------------------------------------------
detected_objects_pub.publish(detected_objects)
Following image showing the objects with predicted names:
Last part of pcl_callback()
function is to call the PR2 mover to pick and place detected objects.
if len(detected_objects)>0:
try:
pr2_mover(detected_objects)
except rospy.ROSInterruptException:
pass
else:
rospy.logwarn('No detected objects !!!')
First step in mover fuction is to initialize variables including ROS messages.
test_scene_num = Int32()
object_name = String()
pick_pose = Pose()
place_pose = Pose()
arm_name = String()
yaml_dict_list = []
# Update test scene number based on the selected test.
test_scene_num.data = 3
read objects list and drop box data from ROS parameters server.
object_list_param = rospy.get_param('/object_list')
dropbox_param = rospy.get_param('/dropbox')
This is to rotate PR2 to capture side tables data to avoid collision. This can be further enhanced as mentioned in last section of project text.
# Rotate Right
pr2_base_mover_pub.publish(-1.57)
rospy.sleep(15.0)
# Rotate Left
pr2_base_mover_pub.publish(1.57)
rospy.sleep(30.0)
# Rotate Center
pr2_base_mover_pub.publish(0)
here we will calculate the centroid (x,y,z) of each detected object based on its points array.
labels = []
centroids = [] # to be list of tuples (x, y, z)
for object in object_list:
labels.append(object.label)
points_arr = ros_to_pcl(object.cloud).to_array()
centroids.append(np.mean(points_arr, axis=0)[:3])
in this loop we will be picking each object from the pick-list we received through ROS parameter server and match it to one of the detected objects to decide on pick pose, place pose, and arm name. We will write all date to yaml file.
for i in range(0, len(object_list_param)):
# Read object name and group from object list.
object_name.data = object_list_param[i]['name' ]
object_group = object_list_param[i]['group']
# Select pick pose
try:
index = labels.index(object_name.data)
except ValueError:
print "Object not detected: %s" %object_name.data
continue
pick_pose.position.x = np.asscalar(centroids[index][0])
pick_pose.position.y = np.asscalar(centroids[index][1])
pick_pose.position.z = np.asscalar(centroids[index][2])
# Select place pose
position = search_dictionaries('group', object_group, 'position', dropbox_param)
place_pose.position.x = position[0]
place_pose.position.y = position[1]
place_pose.position.z = position[2]
# Select the arm to be used for pick_place
arm_name.data = search_dictionaries('group', object_group, 'name', dropbox_param)
# Create a list of dictionaries for later output to yaml format
yaml_dict = make_yaml_dict(test_scene_num, arm_name, object_name, pick_pose, place_pose)
yaml_dict_list.append(yaml_dict)
# Wait for 'pick_place_routine' service to come up
rospy.wait_for_service('pick_place_routine')
try:
pick_place_routine = rospy.ServiceProxy('pick_place_routine', PickPlace)
# Insert your message variables to be sent as a service request
resp = pick_place_routine(test_scene_num, object_name, arm_name, pick_pose, place_pose)
print ("Response: ",resp.success)
except rospy.ServiceException, e:
print "Service call failed: %s"%e
file will be automatically named based on the selected test number (1-3).
yaml_filename = 'output_'+str(test_scene_num.data)+'.yaml'
send_to_yaml(yaml_filename, yaml_dict_list)
Following code is to create all required ROS node, subscribers, and publishers.
if __name__ == '__main__':
#----------------------------------------------------------------------------------
# ROS node initialization
#----------------------------------------------------------------------------------
rospy.init_node('clustering', anonymous=True)
#----------------------------------------------------------------------------------
# Create Subscribers
#----------------------------------------------------------------------------------
pcl_sub = rospy.Subscriber("/pr2/world/points", pc2.PointCloud2, pcl_callback, queue_size=1)
#----------------------------------------------------------------------------------
# Create Publishers
#----------------------------------------------------------------------------------
pcl_static_out_pub = rospy.Publisher("/pcl_static_out", PointCloud2, queue_size=1)
pcl_vox_pub = rospy.Publisher("/pcl_vox", PointCloud2, queue_size=1)
pcl_pass_through_pub = rospy.Publisher("/pcl_pass_through", PointCloud2, queue_size=1)
pcl_objects_pub = rospy.Publisher("/pcl_objects", PointCloud2, queue_size=1)
pcl_table_pub = rospy.Publisher("/pcl_table", PointCloud2, queue_size=1)
pcl_cluster_pub = rospy.Publisher("/pcl_cluster", PointCloud2, queue_size=1)
# Publisher for detected object with markers,,,,,,,,,,,,,,,,,
object_markers_pub = rospy.Publisher("/object_markers", Marker, queue_size=100)
detected_objects_pub = rospy.Publisher("/detected_objects", DetectedObjectsArray, queue_size=1)
# Initialize color_list
get_color_list.color_list = []
#----------------------------------------------------------------------------------
# Load Model From disk
#----------------------------------------------------------------------------------
model = pickle.load(open('model.sav', 'rb'))
clf = model['classifier']
encoder = LabelEncoder()
encoder.classes_ = model['classes']
scaler = model['scaler']
#----------------------------------------------------------------------------------
# Spin while node is not shutdown
#----------------------------------------------------------------------------------
while not rospy.is_shutdown():
rospy.spin()
#----------------------------------------------------------------------------------
Next we will be using the above mentioned pipeline to test all of the three worlds. We select the required test world by changing the following lines in pick_place_project.launch
<!--TODO:Change the world name to load different tabletop setup-->
<arg name="world_name" value="$(find pr2_robot)/worlds/test1.world"/>
and
<!--TODO:Change the list name based on the scene you have loaded-->
<rosparam command="load" file="$(find pr2_robot)/config/pick_list_1.yaml"/>
Results are as following:
Test 1 | Values |
---|---|
Features in Training Set: | 480 |
Invalid Features in Training set: | 0 |
Scores: | [0.9375 0.85416667 0.92708333 0.875 0.92708333] |
Accuracy: | 0.90 (+/- 0.07) |
accuracy score: | 0.9041666666666667 |
image of predicted objects:
The output yaml files are on the following links:
-
When compiling using catkin_make I used to get error "cannot convert to bool". I resolved it by adding
static_cast<bool>()
. see this -
Robot was not grasping the detected objects properly in many of the cases although the arm approach is correct and grasper is closing properly. I believe this is related to the setting of grasp close position.
-
Collison avoidance need to be done as discribed in project last section. If I have more time I will work on it.
-
We can go through the object detection pipline once after everytime we pick an object, this will give better results in crowded table case like test 3.
-
PCL documentation : http://strawlab.github.io/python-pcl/
-
RANSAC algorithm : http://homepages.inf.ed.ac.uk/rbf/CVonline/LOCAL_COPIES/FISHER/RANSAC/
-
Outlier Removal (paper) : http://people.csail.mit.edu/changil/assets/point-cloud-noise-removal-3dv-2016-wolff-et-al.pdf
-
Clustering Algorithm : http://bit.ly/clustering-tutorial
-
Segmentation with NN (intro) : http://bit.ly/segmentation-intro-nn
**# Mars Rover Society, IIITDM Kancheepuram**