1. Introduction

2. Observations

3. Results
3.1. Emission components and characteristics of line profiles
3.2. Observed parameters
3.3. Derived physical parameters
3.4. Mapping results

4. Discussion
4.1. The line center velocities
4.2. Distances of the clumps
4.3. Physical Parameter distributions in the Galaxy
4.4. Line profiles
4.5. Conditions of the clumps at high latitude clumps
4.6. States of the ten mapped clumps
4.7. Gas and dust coupling
4.8. Evolutionary phases - A comparison to different star formation samples

5. Summary